A dataset provided by the European Space Agency

Name 011119
Title X-ray Spectroscopy of the Early-Type Elliptical Galaxy NGC4636
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111190101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111190201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111190501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111190701

DOI https://doi.org/10.5270/esa-kt89qbt
Author European Space Agency
Description GT - NGC 4636 is one of the brightest early-type elliptical galaxies. Studying
the extended X-ray emission from the interstellar medium (ISM) of early-type
galaxies is an important way to understand the evolution of these galaxies. ASCA
and ROSAT observations have yielded unexpected, yet sometimes controversial,
sub-solar metal abundances for the ISM of these galaxies. We propose a 100 ksec
observation of NGC 4636 using the RGS as the primary instrument. It will
perform high-resolution spectroscopy and determine the temperature distribution
and chemical abundances of the X-ray emitting plasma. The EPICs in full window
mode with the medium filter will be used to perform spatially-resolved
spectroscopy.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-07-13T00:16:27Z/2001-01-06T04:38:00Z
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 2002-12-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002, X-Ray Spectroscopy Of The Early-Type Elliptical Galaxy Ngc4636, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-kt89qbt