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相关论文: Spatially resolved X-ray spectra of NGC 4258

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XMM-Newton observed the Seyfert 1.9 galaxy NGC 4258 in December 2000. At energies above 2 keV a hard nuclear point source is resolved that can be fitted by a highly absorbed power-law spectrum (NH = (8.0+-0.4)x10^22 cm^-2, photon index…

天体物理学 · 物理学 2009-11-07 W. Pietsch , A. M. Read

We report sub-arcsecond resolution X-ray imaging spectroscopy of the low luminosity active galactic nucleus of NGC 4258 and its immediate surroundings with the Chandra X-ray Observatory. NGC 4258 was observed four times, with the first two…

天体物理学 · 物理学 2009-11-10 A. J. Young , A. S. Wilson

This paper presents high resolution X-ray observations with Chandra of NGC 4258 and infers the nature of the so called ``anomalous arms'' in this galaxy. The anomalous arms dominate the X-ray image; diffuse X-ray emission from the…

天体物理学 · 物理学 2009-11-06 A. S. Wilson , Y. Yang , G. Cecil

We utilize the complimentary capabilities of XMM-Newton and Chandra, to conduct a detailed imaging and spectral study of the nearby galaxy NGC 4945 focussing on its nucleus and immediate surroundings (within ~1 kpc of the nucleus). A…

天体物理学 · 物理学 2016-08-30 N. J. Schurch , T. P. Roberts , R. S. Warwick

We present a deep X-ray observation of the low-luminosity active galactic nucleus in NGC4258 (M106) using ASCA. The soft X-ray spectrum <2keV is dominated by thermal emission from optically-thin plasma with kT~0.5keV. The hard X-ray…

天体物理学 · 物理学 2009-10-31 C. S. Reynolds , M. A. Nowak , P. R. Maloney

We present new X-ray observations of the nucleus, jet and extended emission of the nearby radio galaxy NGC 6251 using the Chandra/ACIS-S camera, together with a reanalysis of archival Chandra/ACIS-I and XMM-Newton/EPIC data. We find that…

天体物理学 · 物理学 2009-11-10 D. A. Evans , M. J. Hardcastle , J. H. Croston , D. M. Worrall , M. Birkinshaw

We present the first results from an XMM-Newton observation of the FRI galaxy NGC 4261, which harbors a supermassive black hole and a low-ionization nuclear emission-line region (LINER). Here we focus on the X-ray properties of the nucleus,…

天体物理学 · 物理学 2009-11-07 R. M. Sambruna , M. Gliozzi , M. Eracleous , W. N. Brandt , R. Mushotzky

We present an XMM observation of the radio jet and diffuse halo of the nearby radio galaxy NGC6251. The EPIC spectrum of the galaxy's halo is best-fitted by a thermal model with temperature kT~1.6 keV and subsolar abundances. Interestingly,…

天体物理学 · 物理学 2009-11-10 R. M. Sambruna , M. Gliozzi , D. Donato , F. Tavecchio , C. C. Cheung , R. Mushotzky

We present Chandra X-ray observations of the nearby Seyfert 1.5 galaxy NGC 4151. The images show the extended soft X-ray emission on the several hundreds of pc scale with better sensitivity than previously obtained. The spectrum of the…

天体物理学 · 物理学 2009-11-07 Y. Yang , A. S. Wilson , P. Ferruit

We report on the nuclear X-ray properties of the radio galaxy NGC 6251 observed with XMM-Newton. NGC 6251 is a well-known radio galaxy with intermediate FRI/II radio properties. It is optically classified as a Seyfert 2 and hosts a…

天体物理学 · 物理学 2009-11-10 M. Gliozzi , R. M. Sambruna , W. N. Brandt , R. Mushotzky , M. Eracleous

BeppoSAX observed NGC4258 on December 1998, when its 2-10 keV luminosity was \~1E41 erg/s. 100% variability is observed in the 3-10 keV band on timescales of a half a day while 20% variability is observed on timescales of one hour. The…

We detect widespread [CII]157.7um emission from the inner 5 kpc of the active galaxy NGC 4258 with the SOFIA integral field spectrometer FIFI-LS. The emission is found associated with warm H2, distributed along and beyond the end of…

The nearby low-luminosity active galactic nucleus (LLAGN) NGC 4258 has a weak radio continuum component at the galactic center. We investigate its radio spectral properties on the basis of our new observations using the Nobeyama Millimeter…

星系天体物理 · 物理学 2015-06-12 Akihiro Doi , Kotaro Kohno , Kouichiro Nakanishi , Seiji Kameno , Makoto Inoue , Kazuhiro Hada , Kazuo Sorai

We have examined X-ray and optical observations of two ultra-luminous X-ray sources, X7 and X10 in NGC4559, using XMM-Newton, Chandra and HST. The UV/X-ray luminosity of X7 exceeds 2.1e40 erg/s in the XMM-Newton observation, and that of X10…

We present high-resolution soft-X-ray spectra of the prototypical Seyfert 2 galaxy, NGC 1068, taken with XMM-Newton RGS and Chandra LETGS. Its rich emission-line spectrum is dominated by recombination in a warm plasma (bright, narrow…

We present a Spitzer Infrared Spectrograph (IRS) map of H2 emission from the nearby galaxy NGC 4258 (Messier 106). The H2 emission comes from 9.4E6 Msun of warm molecular hydrogen heated to 240-1040 K in the inner anomalous arms, a…

星系天体物理 · 物理学 2015-06-19 Patrick M. Ogle , Lauranne Lanz , Philip N. Appleton

We report on a new XMM-Newton observation of NGC 247 from December 2009. The galaxy contains a supersoft, ultraluminous X-ray source (ULX) whose spectrum consists of a thermal component with a temperature about 0.1 keV and a power-law tail…

高能天体物理现象 · 物理学 2015-05-27 Jing Jin , Hua Feng , Philip Kaaret , Shuang-Nan Zhang

We present integral field spectroscopic observations of the central region of the active galaxy NGC 4258 obtained with the fibre IFU system INTEGRAL. We have been able to detect cold neutral gas by means of the interstellar NaD doublet…

星系天体物理 · 物理学 2015-05-18 J. Jiménez-Vicente , E. Mediavilla , A. Castillo-Morales , E. Battaner

We present a Chandra ACIS-S observation of the nuclear region of the nearby spiral galaxy M51 (NGC 5194), which has a low-luminosity Seyfert 2 nucleus. The X-ray image shows the nucleus, southern extranuclear cloud, and northern loop, the…

天体物理学 · 物理学 2009-11-06 Yuichi Terashima , Andrew S. Wilson

We present results from a 25 ksec CHANDRA ACIS-S observation of galaxies NGC4438 and NGC4435 in the Virgo Cluster. X-ray emission in NGC4438 is observed in a ~700 pc nuclear region, a 2.3 kpc spherical bulge, and a network of filaments…

天体物理学 · 物理学 2009-11-10 Marie E. Machacek , Christine Jones , William R. Forman
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