A dataset provided by the European Space Agency

Name: X-ray emission from the PN Abell 30 and its born-again central star
Published: 2010-11-21T00:00:00Z

Proposal ID	060536
Title	X-ray emission from the PN Abell 30 and its born-again central star
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605360101
DOI	https://doi.org/10.5270/esa-f1wybzf
Principal Investigator, PI	Dr Wolf-Rainer Hamann
Abstract	We propose to secure a 50 ksec exposure with XMM-Newton of the Planetary NebulaAbell30. This PN has a hydrogen-deficient central star of WC-PG1159 transitiontype and fits into the born-again scenario. We expect to detect at least1000 X-ray counts from the hot bubble, that will allow us to address thephysics of the hot bubbles inside Planetary Nebulae, and in particular therole of heat conduction for explaining their surprisingly low electrontemperature. The analysis of EPIC spectra will also allow to investigateevolutionary origin of hydrogen-deficient post-AGB stars, in particular to checkthe validity of the born-again scenario.
Publications	Rebirth of X-Ray Emission from the Born-again Planetary Nebula A30 \|Guerrero M. A. Ruiz N. et al. \| ApJ \| 755-129 \| 2012 \| 2012ApJ...755..129G \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...755..129G 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 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 Carbon dust in the evolved born-again planetary nebulae A 30 and A 78 \|Toalu00e1 J. A. Jimu00e9nez-Hernu00e1ndez P. et al. \| MNRAS \| 503-1543 \| 2021 \| 2021MNRAS.503.1543T \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.1543T 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	2009-10-21T19:08:37Z/2009-10-22T11:17:50Z
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	2010-11-21T00:00:00Z
Last Update	2025-01-27
Keywords	"'' scenario", "evolutionary origin", "EPIC", "epic spectra", "xmm newton", "XMM-Newton", "planetary nebula abell30", "scenario ''.", "heat conduction", "x ray emission", "central star", "`` born", "pn abell", "xray counts", "XMM", "Abell 30"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Wolf-Rainer Hamann, 2010, 'X-ray emission from the PN Abell 30 and its born-again central star', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f1wybzf