A dataset provided by the European Space Agency

Name: The X-ray Emission of Late-type Companions to Planetary Nebula Nuclei
Published: 2008-05-30T00:00:00Z

Proposal ID	040167
Title	The X-ray Emission of Late-type Companions to Planetary Nebula Nuclei
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0401670201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0401670301
DOI	https://doi.org/10.5270/esa-jwx0vlw
Principal Investigator, PI	Dr Kevin Briggs
Abstract	Rapid rotation generates strong magnetic activity in late-type stars via adynamo. Late-type companions to the nuclei of planetary nebulae (PNe) areexpected to be rapid rotators due to accretion from the slow heavy wind of thenucleus while it was an AGB star, and hence strong X-ray emitters. Yet,XMM-Newton found two of three such stars to have X-ray activity levels an orderof magnitude lower than those of other fast rotators. This impacts on ourunderstanding of unresolved X-ray sources in PNe and may give clues as to thevital ingredients for an efficient dynamo. We aim to measure the X-ray emissionlevel of the archetype, Abell 35, and the two brightest d symbiotics, young PNecontaining late-type rapid rotators, to test the ubiquity of this low activity.
Publications	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 Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra \|Nunez N. E. Luna G. J. M. et al. \| A&A \| 565-82 \| 2014 \| 2014A&A...565A..82N \| http://ui.adsabs.harvard.edu/#abs/2014A&A...565A..82N 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 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 A D-type symbiotic binary in the planetary nebula SMP LMC 88 \|Ilkiewicz Krystian Mikolajewska Joanna et al. \| MNRAS \| 476-2605 \| 2018 \| 2018MNRAS.476.2605I \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.476.2605I 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 A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 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 X-rays from planetary nebulae: Unveiling wind collisions and binarity \|Montez Rodolfo Jr. \| PhDT \| 0-300 \| 2010 \| 2010PhDT.......300M \| http://ui.adsabs.harvard.edu/#abs/2010PhDT.......300M Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2007-03-15T16:23:09Z/2007-04-30T09:03:56Z
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	2008-05-30T00:00:00Z
Last Update	2026-03-04
Keywords	"agb star", "rapid rotation generates", "efficient dynamo", "magnitude lower", "unresolved xray sources", "xray activity levels", "fast rotators", "magnetic activity", "XMM-Newton", "xray emitters", "xray emission level", "low activity", "xray emission", "vital ingredients", "rapid rotators", "slow heavy wind", "xmm newton", "Abell 35", "late type companions", "XMM", "planetary nebulae pne", "planetary nebula nuclei"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Kevin Briggs, 2008, 'The X-ray Emission of Late-type Companions to Planetary Nebula Nuclei', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jwx0vlw