GT - We propose to measure the parameters of the absorption feature at virgul600 eVoriginally detected by the Einstein SSS in 1H1219+301. Sharp absorption featuresappear to be common in the soft X-ray spectra of BL Lac objects, as shown byseveral detections made with BBXRT: the lines are generally attributed toblue-shifted Lyman alpha OVIII resonance absorption, implying rapid mass outflowfrom the active nucleus. However, the exact nature and origin of these featuresis still unclear. The RGS will provide an accurate measure of the line energyand width, of the column density and the ionisation level of the gas, ultimatelygiving clues to the origin of the gas itself.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2001-06-11T15:24:31Z/2001-06-11T23:43:35Z
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.
European Space Agency, Dr Bert Brinkman, 2002, 'X-ray spectroscopy of the BL Lac 1H1219+301', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6d5dfoe
