| Proposal ID | 020013 |
| Title | THE FORMATION AND EVOLUTION OF X-RAY BINARIES IN ELLIPTICAL GALAXIES |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200130101 |
| DOI | https://doi.org/10.5270/esa-zlmsr4c |
| Principal Investigator, PI | Dr THOMAS MACCARONE |
| Abstract | We propose a 100 ksec observation of NGC 4472 to study the globular cluster(GC)-X-ray binary connection over a large field of view. These data will beespecially useful for comparing the X-ray properties of metal rich and metalpoor globular clusters and for comparing the spatial profiles of cluster andnon-cluster sources. Wide field data are key because metal poor clusters arerare in the inner regions of galaxies and because different spatial profiles arepredicted depending on whether non-GC XRBs are formed in the field or in GCs andthen ejected. The broadband spectroscopy will allow testing of stellar windmodels for the spectral differences as a function of metallicity. We will alsosearch for eclipses to measure orbital periods. |
| Publications |
|
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2004-01-01T03:07:58Z/2004-01-02T09:58:31Z |
| Version | 17.56_20190403_1200 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2005-01-27T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "inner region", "elliptical galaxy", "gc xrbs", "ngc 4472", "xray binary", "globular cluster", "orbital periods", "stellar wind models", "NGC 4472", "especially useful", "xray properties", "predicted depending", "metal rich", "spatial profiles", "broadband spectroscopy", "cluster sources", "wide field data" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr THOMAS MACCARONE, 2005, 'THE FORMATION AND EVOLUTION OF X-RAY BINARIES IN ELLIPTICAL GALAXIES', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zlmsr4c |