Issue |
A&A
Volume 484, Number 2, June III 2008
|
|
---|---|---|
Page(s) | 457 - 461 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20079076 | |
Published online | 08 April 2008 |
Optical and infrared observations of the X-ray source 1WGA J1713.4–3949 in the G347.3-0.5 SNR*
1
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK e-mail: rm2@mssl.ucl.ac.uk
2
INAF - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padua 35122, Italy e-mail: simone.zaggia@oapd.inaf.it
3
INAF - Istituto di Astrofisica Spaziale, via Bassini 15, Milan 20133, Italy e-mail: [deluca;bassan;pat]@iasf-milano.inaf.it
4
JILA and Department of Astrophysical and Planetary Sciences, University of Colorado, 440 UCB, Boulder, 80309, USA e-mail: rosalba@jilau1.Colorado.EDU
Received:
16
November
2007
Accepted:
17
March
2008
Context. X-ray observations unveiled the existence of enigmatic point-like sources at the centre of young supernova remnants (SNRs). These sources, dubbed central compact objects (CCOs), are thought to be neutron stars formed by the supernova explosion. However, their multi-wavelength phenomenology is surprisingly different from that of most young neutron stars.
Aims. The aim of this work is to understand the nature of the CCO 1WGA J1713.4-3949 in the G347.3-0.5 SNR through deep optical and infrared (IR) observations, the first ever performed for this source.
Methods. By exploiting its derived Chandra X-ray position we carried out optical (BVI) observations with the New Technology Telescope (NTT) and adaptive optics IR (JHKs) observations with the Very Large Telescope (VLT).
Results. We detected two faint (,
.) patchy objects close to the Chandra error circle in the NTT images. They were clearly resolved in our
VLT images which unveiled a total of six candidate counterparts
(
) with quite red colours (
~ 0.6). If they
are stars, none of them can be associated with 1WGA J1713.4-3949 for
the most likely values of distance and hydrogen column density. The
identification of the faintest candidate with the neutron star itself
can not be firmly excluded, while the identification with a fallback
disk is ruled out by its non-detection in the I band. No other
candidates are detected down to
,
,
,
21.3, and
20.5.
Conclusions. Our high-resolution IR imaging unveiled a few objects close/within the Chandra X-ray position of 1WGA J1713.4-3949. However, at present none of them can be firmly identified as the object's likely counterpart.
Key words: stars: neutron / stars: individual: 1WGA J1713.4-3949
© ESO, 2008
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.