A dataset provided by the European Space Agency

Name 009441
Title Hot Gas In and Around the Supergiant Shell LMC-2
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094410101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094410201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094410401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094410501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094410601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094410701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094411001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094411101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094411401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0094411501

DOI https://doi.org/10.5270/esa-g0opjk8
Author European Space Agency
Description Supergiant shells with diameters approaching 1000 pc may break through the
gaseous disk of their host galaxy, and transfer energy and mass into the
galactic halo. The Large Magellanic Cloud contains several supergiant shells,
among which LMC\,2 has the most spectacular filamentary shell structure and the
brightest diffuse X-ray emission. The X-ray emission exists within the optical
shell boundary, with an extension beyond the southern shell rim. We propose to
use the EPIC cameras on-board XMM to map LMC2 and its southern extension.
These data will be analyzed in conjunction with our extensive multi-wavelength
datasets in order to study the physical structure of the supergiant shell LMC2
and the role it plays in the global structure of the interstellar medium.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-10-19T17:03:40Z/2002-09-26T05:00:04Z
Version PPS_NOT_AVAILABLE
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 2005-01-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005, Hot Gas In And Around The Supergiant Shell Lmc-2, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-g0opjk8