A dataset provided by the European Space Agency

Name: X-ray Study of Born-Again Planetary Nebulae
Published: 2014-06-18T00:00:00Z

Proposal ID	072115
Title	X-ray Study of Born-Again Planetary Nebulae
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721150101
DOI	https://doi.org/10.5270/esa-0bgfafi
Principal Investigator, PI	Dr Martin Guerrero
Abstract	Mass-loading occurs when a fast, tenuous flow ablates a slow, dense clump,resulting in the mixing of cool material into the hot shocked gas. Mass-loadingexists in many astrophysical settings and affects the X- ray luminosity andtemperature of the hot gas. Chandra and XMM-Newton observations of theborn-again planetary nebula (PN) Abell 30 have revealed a puzzling soft pointsource at the central star and soft diffuse X-rays associated with interactionsbetween the fast stellar wind and H-poor ejecta, where mass- loading andcharge-exchange reactions occur. We request XMM-Newton observations of Abell 78,the only additional well-resolved born-again PN, to confirm the effects ofmass-loading and charge-exchange processes in born-again PNe.
Publications	The Born-again Planetary Nebula A78: An X-Ray Twin of A30 \|Toala J. A. Guerrero M. A. et al. \| ApJ \| 799-67 \| 2015 \| 2015ApJ...799...67T \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...799...67T 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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 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	2013-06-02T14:59:55Z/2013-06-03T07:30:10Z
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	2014-06-18T00:00:00Z
Last Update	2026-03-04
Keywords	"central star", "dense clump", "astrophysical settings", "tenuous flow ablates", "resolved born", "mass loading", "XMM-Newton", "hot shocked gas", "fast stellar wind", "cool material", "xmm newton", "x ray luminosity", "abell 78", "Abell 30", "x ray", "soft diffuse xray", "mass loading exists", "XMM", "charge exchange processes", "planetary nebulae", "mass loading occurs", "hot gas"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Martin Guerrero, 2014, 'X-ray Study of Born-Again Planetary Nebulae', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0bgfafi