| Proposal ID | 011288 |
| Title | X-ray spectra and metal abundances of stars across the H-R diagram |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880101 |
| DOI | https://doi.org/10.5270/esa-l7if11z |
| Principal Investigator, PI | Dr Bernd Aschenbach |
| Abstract | GT- We want to use the XMM EPIC camera to observe a carefully selected sampleof cool stars located on key positions in the H-R diagram, MS and pre-MS stars.The goal of our observations is to obtain good S/N spectra and metal abundancesof one example of each of the different classes of stars. Our observations onAlgol and YY Gem are time-critical for simultaneous observations with Chandra.On Algol and CF Tuc, we request continuous observations centered on a primaryeclipse. On YY Gem, our observation should be continuous, too, to cover thefull orbit. HR 1084 is a calibration target for stray light monitoring with thetransparent filter, but we need to do our GT observation with the thin filter. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2000-07-09T11:30:43Z/2003-01-19T15:28:02Z |
| 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 | 2004-02-20T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "", "pre ms stars", "EPIC", "yy gem", "x ray spectra", "stray light", "primary eclipse", "xmm epic camera", "hr 1084", "calibration target", "thin filter", "key positions", "cool stars located", "transparent filter "", "XMM", "metal abundance", "cf tuc" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Bernd Aschenbach, 2004, 'X-ray spectra and metal abundances of stars across the H-R diagram', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-l7if11z |