Issue |
A&A
Volume 438, Number 3, August II 2005
|
|
---|---|---|
Page(s) | 949 - 955 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20042274 | |
Published online | 18 July 2005 |
A search for very active stars in the Galaxy
First results
1
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia e-mail: gregory.tsarevsky@atnf.csiro.au
2
Astro Space Center, Lebedev Physical Institute, 84/32 Profsoyuznaya St., 117997 Moscow, Russia
3
Isaac Newton Institute of Chile, Moscow Branch, 13 Universitetskij Pr., Moscow 119992, Russia
4
Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France e-mail: thevenin@obs-nice.fr
5
Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia
6
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachaevo-Cherkesia 369167, Russia
7
Sternberg Astronomical Institute, 13 Universitetskij Pr., Moscow 119992, Russia
Received:
28
October
2004
Accepted:
9
February
2005
We report the first results of a systematic search near the plane
of the Galaxy
for so-called very active stars (VAS), which are characterized by a hard X-ray
spectrum and activity in the radio domain.
Candidates with hard X-ray binary-like spectra have been selected
from the Bright ROSAT Source Catalogue in the Zone of Avoidance ()
and were tentatively identified in GB6/PMM/NVSS radio surveys. Most of them were
observed with the ATCA and VLA. Precise radio coordinates have led to unambiguous optical
identification for 60 candidates, and a sub-sample of five of them
has been observed with the VLT.
Also some discovery and confirmatory spectra were obtained with the AAT (4-m) and BTA (6-m).
Spectroscopy with moderate dispersion, made with the FORS1 spectrograph of the VLT
has revealed two stellar objects (one of them, VASC J1628-41, is definitively
a binary VAS), one new AGN and two featureless spectrum sources. One of these objects, VASC J1353-66,
shows marginal evidence of proper motion, which, if confirmed,
would imply the discovery of a new type of galactic source.
Key words: stars: activity
© ESO, 2005
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