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19982026
most citedThe X-ray Source Population of "The Antennae" Galaxies: X-ray Properties from Chandra and Multiwavelength Associations

170 citations · 950 across the 35 of their papers we have counts for

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13 papers · 1 filter

astro-ph2007★ 25 cited

New flaring of an ultraluminous X-ray source in NGC 1365

R. Soria, A. Baldi, G. Risaliti +4

We have studied a highly variable ultraluminous X-ray source (ULX) in the Fornax galaxy NGC 1365, with a series of 12 Chandra and XMM-Newton observations between 2002 and 2006. In…

astro-ph2006★ 28 cited

Probing the Low-Luminosity XLF in Normal Elliptical Galaxies

D. -W. Kim, G. Fabbiano, V. Kalogera +8

We present the first low luminosity (LX > 5 - 10 1036 erg s-1) X-ray luminosity functions (XLFs) of low-mass X-ray binaries (LMXBs) determined for two typical old elliptical galaxi…

astro-ph2004★ 27 cited

Chemical enrichment of the complex hot ISM of the Antennae galaxies: I. Spatial and spectral analysis of the diffuse X-ray emission

A. Baldi, J. C. Raymond, G. Fabbiano +5

We present an analysis of the properties of the hot interstellar medium (ISM) in the merging pair of galaxies known as The Antennae (NGC 4038/39), performed using the deep, coadded…

astro-ph2003★ 18 cited

NGC 4261 and NGC 4697: rejuvenated elliptical galaxies

A. Zezas, L. Hernquist, G. Fabbiano +1

Chandra images present evidence for a non-uniform spatial distribution of discrete X-ray sources in the elliptical galaxy NGC 4261. This non-uniform distribution is inconsistent wi…

astro-ph2003★ 26 cited

Chandra observations of NGC4698: a Seyfert-2 with no absorption

I. Georgantopoulos, A. Zezas

We present Chandra ACIS-S observations of the enigmatic Seyfert-2 galaxy NGC4698. This object together with several other bona-fide Seyfert-2 galaxies show no absorption in the low…

astro-ph2002★ 14 cited

X-ray luminous galaxies I. Chandra observations of IRAS00317-2142

I. Georgantopoulos, A. Zezas, M. J. Ward

We present Chandra observations of the enigmatic galaxy IRAS00317-2142, which is classified as a star-forming galaxy on the basis of the ionization level of its emission lines. How…