| Name | 072232 |
| Title | Accretion, Jets, and a Superhot Corona in the T Tauri Star RY Tau |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722320101 |
| DOI | https://doi.org/10.5270/esa-gcs5yfm |
| Author | European Space Agency |
| Description | We have detected bright X-ray emission from the rapidly-accreting jet-driving T Tauri star RY Tau. Chandra ACIS-S spectra reveal a wealth of emission lines arising in a multi-temperature plasma consisting of a superhot variable component and a very soft component traced down to approximately 0.2 keV. ACIS-S images show faint soft emission extending outward along the jet. We propose to obtain a high-resolution grating spectrum of RY Tau using RGS. The spectrum will provide crucial information needed to construct a detailed emission model and identify the origin of the very soft component, which likely arises at the base of the jet or an accretion shock. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2013-08-21T04:16:33Z/2013-08-22T11:33:13Z |
| Version | 17.56_20190403_1200 |
| 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. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2014-09-11T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2014, Accretion Comma Jets Comma And A Superhot Corona In The T Tauri Star Ry Tau, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gcs5yfm |