[SK2009] X10 , the SIMBAD biblio

2009ApJ...692..443S - Astrophys. J., 692, 443-458 (2009/February-2)

The X-ray point-source population of NGC 1365: the puzzle of two highly-variable ultraluminous X-ray sources.

STRATEVA I.V. and KOMOSSA S.

Abstract (from CDS):

We present 26 point-sources discovered with Chandra within 200'' (~20 kpc) of the center of the barred supergiant galaxy NGC 1365. The majority of these sources are high-mass X-ray binaries, containing a neutron star or a black hole accreting from a luminous companion at a sub-Eddington rate. Using repeat Chandra and XMM-Newton, as well as optical observations, we discuss in detail the natures of two highly variable ultraluminous X-ray sources (ULXs): NGC 1365 X1, one of the most luminous ULXs known since the ROSAT era, which is X-ray variable by a factor of 30, and NGC 1365 X2, a newly discovered transient ULX, variable by a factor of >90. Their maximum X-ray luminosities ((3-5)x1040 erg/s, measured with Chandra) and multiwavelength properties suggest the presence of more exotic objects and accretion modes: accretion onto intermediate mass black holes (IMBHs) and beamed/super-Eddington accretion onto solar-mass compact remnants. We argue that these two sources have black hole masses higher than those of the typical primaries found in X-ray binaries in our Galaxy (which have masses of <20 M), with a likely black-hole mass of 40-60 M in the case of NGC 1365 X1 with a beamed/super-Eddington accretion mode, and a possible IMBH in the case of NGC 1365 X2 with M = 80-500 M.

Abstract Copyright:

Journal keyword(s): galaxies: individual: NGC 1365 - X-rays: binaries - X-rays: galaxies

Nomenclature: Table 1: [SK2009] XNN (Nos X1-X26).

Simbad objects: 33

goto View the reference in ADS


2020.07.09-16:15:49

© Université de Strasbourg/CNRS

    • Contact