Name | 065245 |
Title | Identity of Nuclear X-ray Sources in Bulge-less Galaxies |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652450101 |
DOI | https://doi.org/10.5270/esa-1rvee60 |
Author | Prof Smita Mathur |
Description | We initiated a Chandra program to search for low-level nuclear activity in a representative sample of late-type galaxies within 20 Mpc. We propose XMM-Newton observations of two late-type galaxies, Scd and Sd, in both of which a nuclear X-ray source was detected with Chandra. X-ray spectra and optical-X-ray spectral energy distributions obtained with XMM-Newton will secure the identification of X-ray sources as either AGNs, low-mass X-ray binaries or star clusters. Discovering secure AGNs in these bulge-less galaxies will be exciting as it will imply that bulges are not necessary for existence of black holes. This will have important consequences towards understanding the formation and co-evolution of black holes and galaxies. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2010-07-15T19:08:18Z/2010-07-16T16:40:58Z |
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 | 2011-08-07T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2011-08-07T00:00:00Z, 065245, 17.56_20190403_1200. https://doi.org/10.5270/esa-1rvee60 |