Issue |
A&A
Volume 453, Number 1, July I 2006
|
|
---|---|---|
Page(s) | 295 - 299 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20065025 | |
Published online | 09 June 2006 |
M-type giants as optical counterparts of X-ray sources 4U 1700+24 and 4U 1954+319
1
INAF – Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna, via Gobetti 101, 40129 Bologna, Italy (formerly IASF/CNR, Bologna) e-mail: masetti@iasfbo.inaf.it
2
Dipartimento di Fisica, Università di Ferrara, via Saragat 1, 44100 Ferrara, Italy
Received:
15
February
2006
Accepted:
9
March
2005
We observed with Chandra two peculiar galactic X-ray
sources, 4U 1700+24 and 4U 1954+319, which are suspected to have a
M-type giant star as optical counterpart, in order to get a
high-precision astrometric position for both of them. The peculiarity of
these sources lies in the fact that these are the only two cases among
low-mass X-ray binaries (LMXBs), besides the confirmed case of GX 1+4,
for which the companion can possibly be a M-type giant.
We found that in both cases the field M-type giant star
is indeed the counterpart of these X-ray sources. We also determined
the distance to 4U 1954+319 to be ~1.7 kpc. This result suggests
that a number of faint ( erg s-1) Galactic X-ray sources are “symbiotic X-ray binaries”,
that is, wide-orbit LMXBs composed of a compact object, most likely a
neutron star, accreting from the wind of a M-type giant.
Key words: astrometry / stars: binaries: general / X-rays: binaries / stars: neutron / stars: individuals: 4U 1700+24 / stars: individual: 4U 1954+319
© ESO, 2006
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