
| Proposal ID | 010546 |
| Title | New ROSAT discovered Intermediate Polars in the Galactic Plane TS_30 |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460101 |
| DOI | https://doi.org/10.5270/esa-vd8c7y9 |
| Principal Investigator, PI | Dr Bernd Aschenbach |
| Abstract | GT-XMM observations of newly discovered intermediate polars (IPs) are proposed.Broad band pulse phase resolved spectroscopy will allow to investigate thedifferent emission components observed in the X-ray spectra of IPs. The largecollecting area and high spectral resolution of the EPIC detectors will providehigh quality spectra for a detailed modeling to get insight into the accretionprocess close to the surface of the white dwarf. RXJ1914.4+2456 is of particularinterest. It was proposed as candidate for a soft IP or might be the firstdouble-degenerate polar in which case the 569 s period would indicate theorbital period. We propose a 2nd observation about one year after that ofK. Mason to follow the period history. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2000-09-07T10:02:37Z/2004-10-02T06:21:54Z |
| Version | 21.51_20241115_1113 |
| 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 | 2005-11-01T00:00:00Z |
| Last Update | 2026-07-09 |
| Keywords | "accretion process close", "intermediate polars ips", "intermediate polars", "white dwarf", "spectral resolution", "double degenerate polar", "ROSAT", "soft ip", "epic detectors", "xray spectra", "quality spectra", "emission components", "period history", "galactic plane ts_30", "orbital period", "EPIC", "XMM" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Bernd Aschenbach, 2005, 'New ROSAT discovered Intermediate Polars in the Galactic Plane TS_30', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-vd8c7y9 |
| Rights | Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license. |