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Letter to the Editor
Super-strong X-ray emission from a deeply embedded young stellar object in the Serpens cloud core
Received 21 July 1998 / Accepted 7 August 1998
We report the ROSAT detection of strong X-ray emission from an optically invisible infrared source in the Serpens star forming region. The X-ray source can be identified with the infrared star EC 95, a deeply embedded ( mag) young stellar object. The quiescent soft X-ray luminosity of this object is about erg/sec, making it the most X-ray luminous young stellar object ever detected. Since this exceeds the quiescent, i.e. non-flaring, X-ray luminosity of any known coronal X-ray source by at least about one order of magnitude, our result suggests that a non-solar-like origin for the X-ray emission of EC 95 has to be considered.
Key words: Stars: formation, pre-main sequence, coronae X-rays: stars
Send offprint requests to: T. Preibisch
Online publication: September 8, 1998