AD Leonis: Flares observed by XMM-Newton and Chandra
| dc.creator | Besselaar, E. J. M. van den | |
| dc.creator | Raassen, A. J. J. | |
| dc.creator | Mewe, R. | |
| dc.creator | van der Meer, R. L. J. | |
| dc.creator | Guedel, M. | |
| dc.creator | Audard, M. | |
| dc.date | 2003-09-11 | |
| dc.date.accessioned | 2026-07-07T02:09:31Z | |
| dc.date.available | 2026-07-07T02:09:31Z | |
| dc.description | The M-dwarf AD Leonis has been observed with the Reflection Grating Spectrometers and the European Photon Imaging Camera aboard XMM-Newton and also with the Low Energy Transmission Grating Spectrometer aboard the Chandra X-ray Observatory. In the observation taken with XMM-Newton five large flares produced by AD Leo were identified and only one in the observation taken with Chandra. A quiescent level to the lightcurves is difficult to define, since several smaller flares mutually overlap each other. However, we defined a quasi-steady state outside of obvious flares or flare decays. The spectra from the flare state and the quasi-steady state are analysed separately. From these spectra the temperature structure was derived with a multi-temperature model and with a differential emission measure model. The multi-temperature model was also used to determine the relative abundances of C, N, O, Ne, Mg, Si, S, and Fe. He-like ions, such as O VII and Ne IX, produce line triplets which are used to determine or constrain the electron temperature and electron density of the corresponding ion. During the flare state a higher emission measure at the hottest temperature is found for both XMM-Newton and Chandra observations. The derived abundances suggest the presence of an inverse First Ionization Potential effect in the corona of AD Leo. | |
| dc.description | 8 pages and 7 figures. Accepted for publication in Astronomy & Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309315 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309315 | |
| dc.identifier | Astron.Astrophys. 411 (2003) 587 | |
| dc.identifier | doi:10.1051/0004-6361:20031398 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6461 | |
| dc.subject | Astrophysics | |
| dc.title | AD Leonis: Flares observed by XMM-Newton and Chandra | |
| dc.type | text |