X-ray properties of NGC 300 I. Global properties of X-ray point sources and their optical counterparts
arXiv:astro-ph/0509383 · doi:10.1051/0004-6361:20042162
Abstract
We present X-ray properties of NGC 300 point sources, extracted from 66 ksec of XMM-Newton data taken in 2000 December and 2001 January. A total of 163 sources were detected in the energy range of 0.3-6 kev. We report on the global properties of the sources detected inside the D25 optical disk, such as the hardness ratio and X-ray fluxes, and on the properties of their optical counterparts found in B, V, and R images from the 2.2m MPG/ESO telescope. Furthermore, we cross-correlate the X-ray sources with SIMBAD, the USNO-A2.0 catalog, and radio catalogues.
arXiv commentThere are 14 pages, 8 figures and 2 tables. The article will be published in Astronomy and Astrophysics
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- Optical Spectra of SNR Candidates in NGC 300
- A new luminous supersoft X-ray source in NGC 300
- XMM-Newton observation of the interacting galaxies NGC1512 and NGC1510
- Color-color diagrams as tools for assessment of the variable absorption in high mass X-ray binaries
- Multiwavelength Study of the X-Ray Bright Supernova Remnant N300-S26 in NGC 300
- Discovery of a deep Seyfert-2 galaxy at z = 0.222 behind NGC 300