A dataset provided by the European Space Agency

Name 076330
Title Understanding X-ray Emission from AGN in Low Surface Brightness Galaxies
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763300501

DOI https://doi.org/10.5270/esa-7glpowx
Author Dr Harsha Raichur
Description We propose for XMM-Newton observations of 6 nearby, bulge dominated giant low surface brightness (GLSB) galaxies. They have diffuse stellar disks and massive HI disks but are overall poor in star formation. They are possibly the most dark matter dominated spirals in our nearby universe and yet a significant fraction of them have prominent bulges that host AGN activity. Optical studies indicate that their AGN black hole masses are low compared to their galaxy masses and lie below the M-sigma correlation. Not much is known about the AGN activity and bulge evolution in these galaxies, especially in the X-ray domain. Our proposed XMM-Newton observations will be used to detect and characterize the X-ray properties of these systems.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-10-27T14:28:55Z/2016-02-18T11:19:10Z
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 2017-03-09T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-03-09T23:00:00Z, 076330, 17.56_20190403_1200. https://doi.org/10.5270/esa-7glpowx