A dataset provided by the European Space Agency

Name 011121
Title Non-thermal emission in shell-like supernova remnants SSC_40
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111210101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111210201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111210301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111210401

DOI https://doi.org/10.5270/esa-hzxhfwx
Author European Space Agency
Description GT- The recent discovery of non-thermal emission from the shell-like
supernova remnants SN1006 and RXJ1713.7-3946 has been interpreted as the
first direct evidence of acceleration of cosmic rays in the shock-fronts
of supernova remnants. We propose XMM observations of two shell-like SNRs
to search for similar evidence of non-thermal emission.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-07-28T04:33:57Z/2001-08-28T18:34:34Z
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 2002-11-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002, Non-Thermal Emission In Shell-Like Supernova Remnants Ssc_40, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hzxhfwx