A dataset provided by the European Space Agency

Name: Stellar Mass Loss Versus External Accretion in X-ray Bright Ellipticals
Published: 2004-11-05T00:00:00Z

Proposal ID	014157
Title	Stellar Mass Loss Versus External Accretion in X-ray Bright Ellipticals
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0141570101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0141570201
DOI	https://doi.org/10.5270/esa-8ghsyit
Principal Investigator, PI	Dr Craig Sarazin
Abstract	Observations of N4552, N4125, N1395, and N1600, four X-ray-bright ellipticalgalaxies with extended emission line filaments and dust, will be used to studythe interaction between the hot, X-ray emitting gas and cooler interstellarmaterial. We will determine whether heat conduction into the cooler gas orenergy losses to grains affect the thermal state of the gas. The elementalabundances and gradients in the hot gas will be derived and compared to thestellar values. If the gas results from local stellar mass loss, the abundancesshould be similar. If there is a cooling flow, the abundances at each radiusshould reflect those of stars at larger radii. The RGS will be used to dispersethe central regions of the galaxies and to detect or limit low ionization X-ray lines from cooling gas.
Publications	Elemental Abundances in the X-Ray Gas of Early-Type Galaxies with XMM-Newton and Chandra Observations \|Ji, Jun, Irwin, Jimmy A., et al. \| ApJ \| 696-2252 \| 2009 \| 2009ApJ...696.2252J \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...696.2252J Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton \|Matsushita, K., \| A&A \| 527-134 \| 2011 \| 2011A&A...527A.134M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.134M The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars \|Young, M., Elvis, M., \| ApJ \| 708-1388 \| 2010 \| 2010ApJ...708.1388Y \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...708.1388Y An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan, A. J., Tanvir, N. R., et al. \| Sci \| 333-199 \| 2011 \| 2011Sci...333..199L \| http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L New constraints on the X-ray spectral properties of type 1 active galactic nuclei \|Scott, A. E., Stewart, G. C., et al. \| MNRAS \| 417-992 \| 2011 \| 2011MNRAS.417..992S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.417..992S The x-ray luminous galaxy cluster population at 0.9 < z &lsim; 1.6 as revealed by the XMM-Newton Distant Cluster Project \|Fassbender, R., Bohringer, H., et al. \| NJPh \| 13-125014 \| 2011 \| 2011NJPh...13l5014F \| http://ui.adsabs.harvard.edu/#abs/2011NJPh...13l5014F Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M Gravitational potential and X-ray luminosities of early-type galaxies observed with XMM-Newton and Chandra \|Nagino, R., Matsushita, K., \| A&A \| 501-157 \| 2009 \| 2009A&A...501..157N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...501..157N 2XMM ultraluminous X-ray source candidates in nearby galaxies \|Walton, D. J., Roberts, T. P., et al. \| MNRAS \| 416-1844 \| 2011 \| 2011MNRAS.416.1844W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.416.1844W A Chandra Survey of Early-Type Galaxies. I. Metal Enrichment in the Interstellar Medium \|Humphrey, Philip J., Buote, David A., \| ApJ \| 639-136 \| 2006 \| 2006ApJ...639..136H \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...639..136H A large catalogue of ultraluminous X-ray source candidates in nearby galaxies \|Walton, D. J., Gladstone, J. C., et al. \| AN \| 332-354 \| 2011 \| 2011AN....332..354W \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..354W Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 412-35 \| 2011 \| 2011MNRAS.412L..35S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..35S A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 \|Georgakakis, Antonis, Nandra, K., \| MNRAS \| 414-992 \| 2011 \| 2011MNRAS.414..992G \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F An X-ray view of 82 LINERs with Chandra and XMM-Newton data \|Gonzalez-Martin, O., Masegosa, J., et al. \| A&A \| 506-1107 \| 2009 \| 2009A&A...506.1107G \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1107G The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei \|Scott, A. E., Stewart, G. C., \| MNRAS \| 423-2633 \| 2012 \| 2012MNRAS.423.2633S \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.2633S The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Using the Bright Ultrahard XMM-Newton survey to define an IR selection of luminous AGN based on WISE colours \|Mateos, S., Alonso-Herrero, A., et al. \| MNRAS \| 426-3271 \| 2012 \| 2012MNRAS.426.3271M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426.3271M Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau, F.-X., Motch, C., et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Exploring X-ray and radio emission of type 1 AGN up to z virgul 2.3 \|Ballo, L., Heras, F. J. H., et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B The Fifth Data Release Sloan Digital Sky Survey/XMM-Newton Quasar Survey \|Young, M., Elvis, M., \| ApJS \| 183-17 \| 2009 \| 2009ApJS..183...17Y \| http://ui.adsabs.harvard.edu/#abs/2009ApJS..183...17Y X-ray spectral variability of seven LINER nuclei with XMM-Newton and Chandra data \|Hernandez-Garcia, L., Gonzalez-Martin, O., et al. \| A&A \| 556-47 \| 2013 \| 2013A&A...556A..47H \| http://ui.adsabs.harvard.edu/#abs/2013A&A...556A..47H A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys \|Brightman, M., Silverman, J. D., et al. \| MNRAS \| 433-2485 \| 2013 \| 2013MNRAS.433.2485B \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.433.2485B Uncovering obscured luminous AGN with WISE \|Mateos, S., Alonso-Herrero, A., et al. \| MNRAS \| 434-941 \| 2013 \| 2013MNRAS.434..941M \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..941M Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-type Galaxies by Accreted Cold Gas \|Su, Yuanyuan, Irwin, Jimmy A., \| ApJ \| 766-61 \| 2013 \| 2013ApJ...766...61S \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...766...61S Synapses of active galactic nuclei:. Comparing X-ray and optical classifications using artificial neural networks \|Gonzalez-Martin, O., Diaz-Gonzalez, D., et al. \| A&A \| 567-92 \| 2014 \| 2014A&A...567A..92G \| http://ui.adsabs.harvard.edu/#abs/2014A&A...567A..92G Discovery of O VII line emitting gas in elliptical galaxies \|Pinto, Ciro, Fabian, Andrew C., et al. \| A&A \| 572-8 \| 2014 \| 2014A&A...572L...8P \| http://ui.adsabs.harvard.edu/#abs/2014A&A...572L...8P Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence \|Pinto, Ciro, Sanders, Jeremy S., et al. \| A&A \| 575-38 \| 2015 \| 2015A&A...575A..38P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..38P Obscuration-dependent Evolution of Active Galactic Nuclei \|Buchner, Johannes, Georgakakis, Antonis, et al. \| ApJ \| 802-89 \| 2015 \| 2015ApJ...802...89B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...802...89B Revisiting the relationship between 6 mum and 2-10 keV continuum luminosities of AGN \|Mateos, S., Carrera, F. J., et al. \| MNRAS \| 449-1422 \| 2015 \| 2015MNRAS.449.1422M \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.1422M ERRATUM: The Fifth Data Release Sloan Digital Sky Survey/XMM-Newton Quasar Survey (2009, ApJS, 183, 17) \|Young, M., Elvis, M., \| ApJS \| 185-250 \| 2009 \| 2009ApJS..185..250Y \| http://ui.adsabs.harvard.edu/#abs/2009ApJS..185..250Y Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Do the spectral energy distributions of type 1 active galactic nuclei show diversity? \|Scott, A. E., Stewart, G. C., \| MNRAS \| 438-2253 \| 2014 \| 2014MNRAS.438.2253S \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2253S XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Unveiling the Physics of Low-luminosity AGNs through X-Ray Variability: LINER versus Seyfert 2 \|Hernandez-Garcia, L., Masegosa, J., et al. \| ApJ \| 824-7 \| 2016 \| 2016ApJ...824....7H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...824....7H Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC \|Mernier, F., de Plaa, J., et al. \| A&A \| 592-157 \| 2016 \| 2016A&A...592A.157M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A.157M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models \|Mernier, F., de Plaa, J., et al. \| A&A \| 595-126 \| 2016 \| 2016A&A...595A.126M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A.126M Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 596-101 \| 2016 \| 2016A&A...596A.101P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...596A.101P Optical spectroscopy of candidates for quasars at 3 < z < 5.5 from the XMM-newton X-ray survey. A distant X-ray quasar at z = 5.08 \|Khorunzhev, G. A., Burenin, R. A., et al. \| AstL \| 43-135 \| 2017 \| 2017AstL...43..135K \| http://ui.adsabs.harvard.edu/#abs/2017AstL...43..135K Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>virgul1 and their Galaxy Populations \|Fassbender, Rene, \| PhDT \| 0-116 \| 2008 \| 2008PhDT.......116F \| http://ui.adsabs.harvard.edu/#abs/2008PhDT.......116F Stripped Elliptical Galaxies as Probes of ICM Physics. III. Deep Chandra Observations of NGC 4552: Measuring the Viscosity of the Intracluster Medium \|Kraft, R. P., Roediger, E., et al. \| ApJ \| 848-27 \| 2017 \| 2017ApJ...848...27K \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...848...27K Improved measurements of turbulence in the hot gaseous atmospheres of nearby giant elliptical galaxies \|Ogorzalek, A., Zhuravleva, I., et al. \| MNRAS \| 472-1659 \| 2017 \| 2017MNRAS.472.1659O \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472.1659O CHEERS: The chemical evolution RGS sample \|de Plaa, J., Kaastra, J. S., et al. \| A&A \| 607-98 \| 2017 \| 2017A&A...607A..98D \| http://ui.adsabs.harvard.edu/#abs/2017A&A...607A..98D Solar abundance ratios of the iron-peak elements in the Perseus cluster \|Hitomi Collaboration, Aharonian, Felix, et al. \| Natur \| 551-478 \| 2017 \| 2017Natur.551..478H \| http://ui.adsabs.harvard.edu/#abs/2017Natur.551..478H Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M Diffusion of elements in the interstellar medium in early-type galaxies \|Medvedev, P. S., Sazonov, S. Yu., \| AstL \| 43-285 \| 2017 \| 2017AstL...43..285M \| http://ui.adsabs.harvard.edu/#abs/2017AstL...43..285M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies \|Mernier, F., Werner, N., et al. \| MNRAS \| 480-95 \| 2018 \| 2018MNRAS.480L..95M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480L..95M Enrichment of the Hot Intracluster Medium: Observations \|Mernier, F., Biffi, V., et al. \| SSRv \| 214-129 \| 2018 \| 2018SSRv..214..129M \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214..129M The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z virgul= 1 \|Gonzalez, Anthony H., Gettings, Daniel P., et al. \| ApJS \| 240-33 \| 2019 \| 2019ApJS..240...33G \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..240...33G Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 104 yr \|Ichikawa, Kohei, Ueda, Junko, et al. \| ApJ \| 870-65 \| 2019 \| 2019ApJ...870...65I \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...65I A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw, H. P., Roberts, T. P., et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups \|Liu, Haonan, Pinto, Ciro, et al. \| MNRAS \| 485-1757 \| 2019 \| 2019MNRAS.485.1757L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.1757L A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties Derived from the SED Fitting with Optical, Infrared, and Radio Data \|Toba, Yoshiki, Yamashita, Takuji, et al. \| ApJS \| 243-15 \| 2019 \| 2019ApJS..243...15T \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..243...15T Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background \|Ananna, Tonima Tasnim, Treister, Ezequiel, et al. \| ApJ \| 889-17 \| 2020 \| 2020ApJ...889...17A \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...889...17A Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B The Metal Content of the Hot Atmospheres of Galaxy Groups \|Gastaldello, Fabio, Simionescu, Aurora, et al. \| Univ \| 7-208 \| 2021 \| 2021Univ....7..208G \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..208G Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z X-ray shapes of elliptical galaxies and implications for self-interacting dark matter \|McDaniel, A., Jeltema, T., \| JCAP \| 5-20 \| 2021 \| 2021JCAP...05..020M \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...05..020M An XMM-Newton Early-type Galaxy Atlas \|Islam, Nazma, Kim, Dong-Woo, et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I High-resolution X-ray spectroscopy of astrophysical plasmas with X-ray microcalorimeters \|Ezoe, Yuichiro, Ohashi, Takaya, \| RvMPP \| 5-4 \| 2021 \| 2021RvMPP...5....4E \| http://ui.adsabs.harvard.edu/#abs/2021RvMPP...5....4E The impact of precession on the observed population of ULXs \|Khan, Norman, Middleton, Matthew J., et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). XII. Ionised gas emission in the inner regions of lenticular galaxies \|Boselli, A., Fossati, M., et al. \| A&A \| 659-46 \| 2022 \| 2022A&A...659A..46B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..46B The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows, R., Comerford, Julia M., et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W Hard X-Ray to Radio Multiwavelength SED Analysis of Local U/LIRGs in the GOALS Sample with a Self-consistent AGN Model including a Polar-dust Component \|Yamada, Satoshi, Ueda, Yoshihiro, et al. \| ApJS \| 265-37 \| 2023 \| 2023ApJS..265...37Y \| http://ui.adsabs.harvard.edu/#abs/2023ApJS..265...37Y The infalling elliptical galaxy M89: the chemical composition of the AGN disturbed hot atmosphere \|Kara, Sinancan, Pl\\u0161ek, Tom\\u00e1\\u0161, et al. \| MNRAS \| 528-1500 \| 2024 \| 2024MNRAS.528.1500K \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528.1500K From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2003-07-10T09:27:28Z/2003-10-17T23:31:17Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2004-11-05T00:00:00Z
Keywords	"hot gas", "heat conduction", "stellar values", "cooling gas", "emission line filaments", "xray emitting gas", "elemental abundance", "cooler interstellar material", "xray bright ellipticals", "cooler gas", "larger radii", "central region", "stellar mass loss", "grains affect", "external accretion", "energy losses", "cooling flow"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Craig Sarazin, 2004, 'Stellar Mass Loss Versus External Accretion in X-ray Bright Ellipticals', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8ghsyit