A dataset provided by the European Space Agency

Name 080478
Title The SNR G160.9+2.6 blast wave interaction with the star forming region Sh-219
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804780101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804780201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804780301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804780401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804780501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804780601

DOI https://doi.org/10.5270/esa-d3wov44
Author Dr Patrick Kavanagh
Description As core collapse supernovae often occur close to their parent molecular clouds, it is expected that interactions between core collapse supernova remnants (SNRs) and young stellar objects (YSOs) forming in those clouds are common. To date virgul40 SNR-molecular cloud associations have been confirmed. SNR shock waves impact the evolution of local YSOs which has implications for star-planet formation. It is important to correctly map the progression of an SNR blast wave through a star-forming region (SFR), assess the impact of the SNR on the SFR, and vice versa. We aim to perform such a study for the case of the SNR G160.9+2.6 interaction with Sh-219.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-03-10T12:48:26Z/2017-03-28T17:47:47Z
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 2018-05-10T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2018-05-10T22:00:00Z, 080478, 17.56_20190403_1200. https://doi.org/10.5270/esa-d3wov44