An X-ray flare detected on the M8 dwarf VB 10

被引：64

作者：

Fleming, TA ^{[1
]}

Giampapa, MS

Schmitt, JHMM

机构：

[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[2] Natl Opt Astron Observ, Natl Solar Observ, Tucson, AZ 85726 USA

[3] Univ Hamburg, Hamburg, Germany

来源：

ASTROPHYSICAL JOURNAL | 2000年 / 533卷 / 01期

关键词：

stars : coronae; stars; low-mass; brown dwarfs; X-rays : stars;

D O I：

10.1086/308657

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have detected an X-ray hare on the very low mass star VB 10 (GL 752 B; M8V) using the ROSAT High Resolution Imager. VB 10 is the latest type (lowest mass) main-sequence star known to exhibit coronal activity. X-rays were detected from the star during a single 1.1 ks segment of an observation that lasted 22 ks in total. The energy released by this flare is on the order of 10(27) ergs s(-1). This is at least 2 orders of magnitude greater than the quiescent X-ray luminosity of VB 10, which has yet to be measured. This X-ray flare is very similar in nature to the far-ultraviolet flare that was observed by Linsky et al. using the Goddard High Resolution Spectrograph onboard the Hubble Space Telescope. We discuss reasons for the extreme difference between the flare and quiescent X-ray luminosities, including the possibility that VB 10 has no quiescent (10(6) K) coronal plasma at all.

引用

页码：372 / 377

页数：6

共 21 条

[1] X-RAY-EMISSION AT THE LOW-MASS END - RESULTS FROM AN EXTENSIVE EINSTEIN-OBSERVATORY SURVEY [J].