|Title||The nature of nuclear X-ray sources in nearby late-type galaxies|
|Author||Prof Smita Mathur|
|Description||We initiated a Chandra program to search for low-level nuclear activity in a representative sample of low-mass galaxies within 20 Mpc. We propose XMM-Newton observations of three late-type galaxies, Sdm-Sc-Sbc, in each 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 identification of X-ray sources as either AGNs, binaries or star clusters. We will understand characteristics of low luminosity AGNs, if present. Discovering AGNs in 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 toward understanding the formation and co-evolution of galaxies and black holes.|
|Publication||No observations found associated with the current proposal|
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2010-07-30T00:00:00Z, 060292, 17.56_20190403_1200. https://doi.org/10.5270/esa-r7pnwgf|