Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...349l..21h&link_type=abstract
Astronomy and Astrophysics, v.349, p.L21-L24 (1999)
Astronomy and Astrophysics
Astrophysics
2
Galaxy: Center, X-Rays: General, X-Rays: Stars
Scientific paper
We have observed the region centered on the hard X-ray transient EXS 1727.9-2952 near the Galactic Centre using the Narrow Field Instruments (NFI) of the BeppoSAX X-ray satellite. The soft X-ray intensity distribution in the full field of the MECS instruments revealed the existence of 10 sources. Three of them are within the 10' error circle of the EXS 1737.9-2952 nominal position. With a 3' flux collection radius, the individual background-subtracted source count rates were 0.0069-0.0162 cts/s with the MECS 2 and 3 data combined, indicating source flux densities of the order 10(-12) erg cm(-2) s(-1) (1.65-10.5 keV). The non-detections in LECS observations indicate that the sources are very weak in the 0.1-2 keV energy range. The locations of the new sources overlap partly with that of the CO molecular cloud observed by us with the SEST telescope at ESO. A few of the new sources are close to the VLA radio sources previously found inside the EXITE error circle of the EXS position, but none of them coincide.
Durouchoux Ph.
Hannikainen Diana
Huovelin Juhani
Muhli Panu
Schultz Jussi
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