A dataset provided by the European Space Agency

Name: X-Raying the Stream/Disk Impact Region in XB1254-69
Published: 2003-02-23T00:00:00Z

Proposal ID	006074
Title	X-Raying the Stream/Disk Impact Region in XB1254-69
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0060740101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0060740501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0060740601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0060740701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0060740801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0060740901
DOI	https://doi.org/10.5270/esa-l5pru2k
Principal Investigator, PI	Dr Duane Liedahl
Abstract	X-ray spectroscopy of LMXB dippers offers the potential to isolate the physics of the collision of the accretion stream with the disk edge, which bears on several aspects of disk accretion. We propose to observe XB1254-69 for three binary orbits (42 ksec). Whether the absorbers are confined to the disk edge orcomprise the denser component of a two-phase medium at smaller radii, in XB1254they are most likely moderately ionized. Using the neutron star as abacklighter, we can infer the physical state of the absorber by measuring edgepositions and depths, and, if the post-impact stream is turbulent, absorptionlines. We have developed sophisticated non-LTE opacity models of 65 ions, withthe expectation that these observations will constrain rad/hydro models of the.
Publications	Discovery of narrow X-ray absorption features from the low-mass X-ray binary X 1254-690 with XMM-Newton \|Boirin, L., Parmar, A. N., \| A&A \| 407-1079 \| 2003 \| 2003A&A...407.1079B \| http://ui.adsabs.harvard.edu/#abs/2003A&A...407.1079B Variations in the dip properties of the low-mass X-ray binary XB 1254-690 observed with XMM-Newton and INTEGRAL \|Diaz Trigo, M., Parmar, A. N., et al. \| A&A \| 493-145 \| 2009 \| 2009A&A...493..145D \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..145D 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 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 Spectral changes during dipping in low-mass X-ray binaries due to highly-ionized absorbers \|Diaz Trigo, M., Parmar, A. N., et al. \| A&A \| 445-179 \| 2006 \| 2006A&A...445..179D \| http://ui.adsabs.harvard.edu/#abs/2006A&A...445..179D 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 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 Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D Interstellar medium composition through X-ray spectroscopy of low-mass X-ray binaries \|Pinto, C., Kaastra, J. S., et al. \| A&A \| 551-25 \| 2013 \| 2013A&A...551A..25P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A..25P Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Oxygen, neon, and iron X-ray absorption in the local interstellar medium \|Gatuzz, Efrain, Garcia, Javier A., et al. \| A&A \| 588-111 \| 2016 \| 2016A&A...588A.111G \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A.111G Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations \|Duro, Refiz, Dauser, Thomas, et al. \| A&A \| 589-14 \| 2016 \| 2016A&A...589A..14D \| http://ui.adsabs.harvard.edu/#abs/2016A&A...589A..14D On the detectability of CO molecules in the interstellar medium via X-ray spectroscopy \|Joachimi, Katerine, Gatuzz, Efrain, et al. \| MNRAS \| 461-352 \| 2016 \| 2016MNRAS.461..352J \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461..352J 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 The composition of the interstellar medium in the Galaxy as seen through X-rays \|Pinto, Ciro, \| PhDT \| 0-3 \| 2013 \| 2013PhDT.........3P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........3P Updating the orbital ephemeris of the dipping source XB 1254-690 and the distance to the source \|Gambino, Angelo F., Iaria, Rosario, et al. \| RAA \| 17-108 \| 2017 \| 2017RAA....17..108G \| http://ui.adsabs.harvard.edu/#abs/2017RAA....17..108G 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 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 The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H 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 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 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	2001-01-22T00:27:12Z/2002-02-08T01:09:49Z
Version	PPS_NOT_AVAILABLE
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	2003-02-23T00:00:00Z
Keywords	"lte opacity models", "post impact stream", "neutron star", "hydro models", "absorption lines", "disk edge", "moderately ionized", "binary orbits", "edge positions", "x raying", "denser component", "accretion stream", "phase medium", "disk impact region", "disk accretion", "lmxb dippers", "constrain rad", "xray spectroscopy", "developed sophisticated"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Duane Liedahl, 2003, 'X-Raying the Stream/Disk Impact Region in XB1254-69', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-l5pru2k