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A&A 411, 509515 (2003) DOI: 10.1051/0004-6361:20031389
 

Summary: A&A 411, 509­515 (2003)
DOI: 10.1051/0004-6361:20031389
c ESO 2003
Astronomy
&
Astrophysics
The X-ray spectra of the flaring and quiescent states
of AT Microscopii observed by XMM-Newton
A. J. J. Raassen1,2, R. Mewe1, M. Audard3, and M. G¨udel4
1
SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
2
Astronomical Institute "Anton Pannekoek", Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
3
Columbia Astrophysics Laboratory, Mail code 5247, 550 West 120th Street, New York, NY 10027, USA
4
Paul Scherrer Institut, W¨urenlingen & Villigen, 5232 Villigen PSI, Switzerland
Received 3 February 2003 / Accepted 29 August 2003
Abstract. The X-ray spectrum of the late-type M-dwarf binary AT Mic (dM4.5e+dM4.5e) is observed in the wavelength range
1­40 Å by means of RGS and EPIC-MOS on board XMM-Newton. During the exposure a flare occured. We have performed a

  

Source: Audard, Marc - INTEGRAL Science Data Centre & Observatory of Geneva, Université de Genève

 

Collections: Physics