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相关论文: A powerful and highly variable off-nuclear X-ray s…

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The nearby barred spiral galaxy NGC 1672 is thought to have a weak Seyfert nucleus in addition to its strong starburst activity. Observations with the PSPC and HRI instruments on board the ROSAT X-ray satellite show that three X-ray sources…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , J. P. Halpern , K. Iwasawa

We report the detection of an absorbed central X-ray source and its strong, rapid variability in NGC4395, the least luminous Seyfert nucleus known. The X-ray source exhibits a number of flares with factors of 3-4 flux changes during a half…

天体物理学 · 物理学 2009-09-17 K. Iwasawa , A. C. Fabian , O. Almaini , P. Lira , A. Lawrence , K. Hayashida , H. Inoue

We present the results of a BeppoSAX observation of the nearby spiral galaxy NGC4945 in the 0.1-200 keV energy band. The nuclear X-ray emission emerges above ~7 keV, through an absorber with column density N_H ~ a few 10^24/cm/cm. Its…

天体物理学 · 物理学 2009-09-25 M. Guainazzi , G. Matt , W. N. Brandt , L. A. Antonelli , P. Barr , L. Bassani

The nearby barred spiral galaxy NGC 1672 shows dramatic starburst activity and may also host a Seyfert 2 nucleus. We present new X-ray observations that set constraints on starburst and Seyfert activity in NGC 1672. Two ROSAT HRI exposures,…

天体物理学 · 物理学 2009-10-31 P. J. de Naray , W. N. Brandt , J. P. Halpern , K. Iwasawa

This paper reports the discovery of a bright X-ray transient source, Suzaku J1305-4913, in the south-west arm of the nearby Seyfert II galaxy NGC 4945. It was detected at a 0.5 -- 10 keV flux of $2.2 \times 10^{-12}$ erg cm$^{-2}$ s$^{-1}$…

We report the Rossi X-ray Timing Explorer observations of the heavily absorbed Seyfert 2 galaxy NGC 4945, which confirm the large column density of the absorber, corresponding to the optical depth to Thomson scattering of about 2.4. The…

天体物理学 · 物理学 2009-10-31 G. M. Madejski , P. T. Zycki , C. Done , A. Valinia , P. Blanco , R. Rothschild , B. Turek

We report the detection of optical and X-ray variability in the least luminous known Seyfert galaxy, NGC4395. The featureless continuum changed by a factor of 2 in 6 months, which is typical of more luminous AGN. The largest variation was…

天体物理学 · 物理学 2009-10-31 P. Lira , A. Lawrence , P. O'Brien , R. A. Johnson , R. Terlevich , N. Bannister

X-ray monitoring observations were performed with the Swift observatory of the ultraluminous X-ray sources Holmberg IX X-1, NGC 5408 X-1, and NGC 4395 X-2 and also of the nuclear X-ray source in NGC 4395. Holmberg IX X-1 remains in the hard…

高能天体物理现象 · 物理学 2015-05-13 Philip Kaaret , Hua Feng

We present new HST NICMOS observations of NGC 4945, a starburst galaxy hosting a highly obscured active nucleus that is one of the brightest extragalactic sources at 100 keV. The HST data are complemented with ground based [FeII] line and…

天体物理学 · 物理学 2007-05-23 A. Marconi , E. Oliva , P. P. van der Werf , R. Maiolino , E. J. Schreier , F. Macchetto , A. F. M. Moorwood

We present a broadband (~0.5-79 keV) spectral and temporal analysis of multiple NuSTAR observations combined with archival Suzaku and Chandra data of NGC4945, the brightest extragalactic source at 100 keV. We observe hard X-ray (> 10 keV)…

We report the optical identifications of two X-ray luminous point sources in the spiral galaxy NGC4565 based on archive data of Chandra and the Hubble Space Telescope. The central X-ray point source, RXJ1236.3+2559, is found to be the…

天体物理学 · 物理学 2009-11-07 H. Wu , S. J. Xue , X. Y. Xia , Z. G. Deng , S. Mao

We report the discovery of a highly polarized millimeter (mm) continuum source in the central region of NGC 4945, identified through ALMA Band 3 observations. This starburst Seyfert 2 galaxy contains numerous compact mm sources, yet only…

We present the results of a 17 ks Chandra ACIS-S observation of the nearby dwarf spiral galaxy NGC 4395. Chandra affords the first high-quality, broadband X-ray detection of the active nucleus of this object that is uncontaminated by nearby…

We present an X-ray spectral and spatial analysis of the composite starburst/Seyfert galaxy NGC 1365. Excellent fits of the ROSAT PSPC spectrum are obtained by combining a soft thermal component with a hard powerlaw. The hard component may…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Hartmut Schulz

In this Paper we report the discovery of CXO J122518.6+144545; a peculiar X-ray source with a position 3.6+-0.2",off-nuclear from an SDSS DR7 z=0.0447 galaxy. The 3.6" offset corresponds to 3.2 kpc at the distance of the galaxy. The 0.3-8…

高能天体物理现象 · 物理学 2015-05-18 P. G. Jonker , M. A. P. Torres , A. C. Fabian , M. Heida , G. Miniutti , D. Pooley

We present the results of Chandra observations of off-nuclear X-ray sources in the spiral galaxy M51 (NGC 5194). 113 X-ray sources have been detected in the field of view and 84 among them project within the disk of NGC 5194. Six and twenty…

天体物理学 · 物理学 2007-05-23 Yuichi Terashima , Andrew S. Wilson

The edge-on spiral galaxy NGC 4565 was observed for $\sim$ 35 ks with ASCA in the 0.5-10 keV energy band. The X-ray emission was dominated by two bright sources, which can be identified with two point-like X-ray sources seen in the ROSAT…

天体物理学 · 物理学 2015-06-24 Tsunefumi Mizuno , Tomohisa Ohnishi , Aya Kubota , Kazuo Makishima , Makoto Tashiro

We report the results of XMM-Newton observations for an especially luminous supersoft X-ray source (SSS) with bolometric luminosity of 10^39 erg/s in the spiral galaxy NGC 300. The source was detected as a SSS in 1992 and disappeared in…

天体物理学 · 物理学 2009-11-07 A. K. H. Kong , R. Di Stefano

We report hints for the correlation between the X-ray and gamma-ray emission in the nearby galaxy NGC 4945, which harbors both an active galactic nucleus and a nuclear starburst region. We have divided the Fermi/LAT observations of NGC 4945…

高能天体物理现象 · 物理学 2017-11-15 Rafal Wojaczynski , Andrzej Niedzwiecki

Six x-ray point sources, with luminosities of $4 \times 10^{38} - 2 \times 10^{39} \rm ergs s^{-1}$ in the 0.4--7 keV band, were detected in Chandra observations of the spiral galaxy M100. One source is identified with supernova SN 1979C…

天体物理学 · 物理学 2009-11-06 Philip Kaaret
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