A dataset provided by the European Space Agency

Name 030186
Title Probing the Environments of Young Supernovae with XMM-Newton


DOI 10.5270/esa-erky4nj
Author Dr Stefan Immler
Description By observing the X-ray emission properties of young supernovae (SNe), physical key parameters such as the circumstellar matter (CSM) density, the mass-loss rate of the progenitor, and the temperature of the outgoing and reverse shock can be studied as a function of time. We propose follow-up observations of the brightest known X-ray emitting SNe (1978K, 1979C, 2004dj) to study the temperature evolution, establish the physical parameters of the ambient CSM out to radii of E18cm from the sites of the explosions, and to monitor the mass-loss rates over 10^4 years in the progenitors stellar wind history. Studying these key parameters as a function of time has never been done before.
Publication Spectral variability of ultraluminous X-ray sources . Kajava, Jari J. E., Poutanen, Juri, . MNRAS . 398-1450 . 2009 . 2009MNRAS.398.1450K ,
X-ray spectral states and metallicity in the ultraluminous X-ray sources NGC 1313 X-1 and X-2 . Pintore, Fabio, Zampieri, Luca, . MNRAS . 420-1107 . 2012 . 2012MNRAS.420.1107P ,
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 ,
XMM-Newton discovery of transient X-ray pulsar in NGC 1313 . Trudolyubov, S. P., . MNRAS . 387-36 . 2008 . 2008MNRAS.387L..36T ,
Multiwavelength Monitoring of the Unusual Ultraluminous Supernova SN 1978K in NGC 1313 and the Search for an Associated Gamma-Ray Burst . Smith, I. A., Ryder, S. D., et all. . ApJ . 669-1130 . 2007 . 2007ApJ...669.1130S ,
Six years of XMM-Newton observations of NGC 1313 X-1 and X-2 . Pintore, F., Zampieri, L., . AN . 332-337 . 2011 . 2011AN....332..337P ,
Associated spectral and temporal state transition of the bright ULXNGC1313 X-1 . Dewangan, G. C., Misra, R., et all. . MNRAS . 407-291 . 2010 . 2010MNRAS.407..291D ,
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 . Lloy...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-10-11T01:02:53Z/2006-03-06T22:46:41Z
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 2008-06-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-06-23T00:00:00Z, 030186, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-erky4nj