A dataset provided by the European Space Agency

Name 030057
Title RGS Observations of the Two X-Ray-Brightest Planetary Nebulae: Origin of Hot Gas
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300570901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571201
...
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300571901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300572901

DOI 10.5270/esa-qod49tm
Author Dr Martin Guerrero
Description Planetary nebulae (PNe) consist of material ejected by stars with masses less than 8-10 solar masses. The current fast stellar wind sweeps up the previous slow AGB wind to form the PN shell, and the shell interior is expected to be filled with hot gas that emits X-rays. Chandra and XMM-Newton have detected diffuse X-rays from PNe at levels much lower than theoretical expectations. The different abundances of the fast stellar wind and the slow AGB wind traces the origin of the hot gas in PNe. We request XMM-Newton RGS observations of the two X-ray-brightest PNe, BD+30 3639 and NGC 6543, to determine the chemical abundances and origin of the hot gas and further use these to constrain the amount of heat conduction between the hot gas and the cool nebular shell.
Publication The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 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 ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift ...
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2006-03-03T23:08:50Z/2006-04-19T02:07:20Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2008-08-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-08-29T00:00:00Z, 030057, 17.56_20190403_1200. https://doi.org/10.5270/esa-qod49tm