A dataset provided by the European Space Agency

Name 030196
Title A search for SN ejecta fragments in a molecular cloud interacting with IC443
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301960101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301960201

DOI 10.5270/esa-natjyaa
Author Dr Fabrizio Bocchino
Description IC443 has been known for a long time as a classical thermal shell. Recently, it has been discovered that it is also a strong source of non-thermal X-ray and gamma-ray radiation. Despite much work has been done which has helped us to better understand this object (detection of an EGRET and BeppoSAX-PDS source, detection of a plerion nebula, detection of a set of hard point sources localized in the region of interaction with a molecular cloud) several issue remains open. With this proposal, we aim to solve one of these issues, the longstanding problem of the nature of the double hard X-ray source 1SAX J0618.0+2227.
Publication XMM-Newton observations of the supernova remnant IC 443. II. Evidence of stellar ejecta in the inner regions . Troja, E., Bocchino, F., et all. . A&A . 485-777 . 2008 . 2008A&A...485..777T ,
On the metal abundances inside mixed-morphology supernova remnants: the case of IC 443 and G166.0+4.3 . Bocchino, F., Miceli, M., . A&A . 498-139 . 2009 . 2009A&A...498..139B ,
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 ,
Isolated X-Ray-Infrared Sources in the Region of Interaction of the Supernova Remnant IC 443 with a Molecular Cloud . Bykov, A. M., Krassilchtchikov, A. M., et all. . ApJ . 676-1050 . 2008 . 2008ApJ...676.1050B ,
INTEGRAL observations of the SNR IC443 region . Bocchino, F., Krassilchtchikov, A. M., et all. . AdSpR . 41-396 . 2008 . 2008AdSpR..41..396B ,
General X-ray properties of hot, massive stars . Naze, Yael, . BSRSL . 80-109 . 2011 . 2011BSRSL..80..109N ,
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...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-03-30T13:25:07Z/2006-03-31T14:01:57Z
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 2007-05-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-05-18T00:00:00Z, 030196, 17.56_20190403_1200. https://doi.org/10.5270/esa-natjyaa