Volume 410, Number 3, November II 2003
|Page(s)||951 - 959|
|Section||Stellar structure and evolution|
|Published online||17 November 2003|
XMM-Newton study of the Serpens star-forming region
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Corresponding author: firstname.lastname@example.org
Accepted: 19 August 2003
We analyze a XMM-Newton X-ray observation of the Serpens dark cloud with a total MOS-equivalent exposure time of 57 ksec. We find 45 individual X-ray sources. None of the class 0 protostars, only one of the class I protostars, and two of the flat-spectrum objects in the region are detected in X-rays. The optically invisible flat-spectrum source EC 95, a very young intermediate mass object, is the strongest X-ray source in the Serpens cloud. The analysis of its X-ray spectrum shows that the hydrogen column density towards EC 95 is considerably lower than expected from the extinction determined from near-IR spectroscopy and photometry. Possible reasons for this inconsistency are discussed.
Key words: open clusters and associations: individual: Serpens dark cloud / stars: formation / stars: coronae / stars: low-mass, brown dwarfs / stars: pre-main sequence / X-rays: stars
© ESO, 2003
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