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相关论文: Chandra Observations of the Mice

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(abridged) High spatial and spectral resolution Chandra X-ray observations of the anomalous merging galaxy NGC520, a similarly-evolved system to the well-known Antennae galaxies, are presented here. Of great interest is the fact that…

天体物理学 · 物理学 2009-11-10 A. M. Read

(abridged) We present a comprehensive comparison of the X-ray properties of a sample of eight dwarf starburst galaxies observed with Chandra (I Zw 18, VII Zw 403, NGC 1569, NGC 3077, NGC 4214, NGC 4449, NGC 5253, He 2-10). In Paper I we…

天体物理学 · 物理学 2009-11-10 Juergen Ott , Fabian Walter , Elias Brinks

We present Chandra observations of two star-forming galaxies (M82 and the Antennae) and three starburst/AGN composite galaxies (NGC1808, NGC6240, NGC7331). In both star-forming galaxies we detect a large number of sources with diverse…

天体物理学 · 物理学 2016-08-30 A. Zezas , G. Fabbiano , A. Prestwich , M. Ward , S. Murray

The superb spatial resolution of Chandra is utilized to study the X-ray morphology of the dwarf starburst galaxy NGC1800 embedded in a small group of galaxies. Diffuse galactic emission is detected, extending several kpc above the galactic…

天体物理学 · 物理学 2009-11-10 Jesper Rasmussen , Ian R. Stevens , Trevor J. Ponman

Arcsecond-resolution X-ray imaging of the nucleus of the nearby starburst galaxy NGC 253 with Chandra reveals a well-collimated, strongly limb-brightened, kiloparsec-scale conical outflow from the central starburst region. The outflow is…

天体物理学 · 物理学 2009-10-31 David K. Strickland , Timothy M. Heckman , Kimberly A. Weaver , Michael Dahlem

Chandra is revolutionising our understanding of the X-ray emission from spiral galaxies. Before Chandra, detailed extragalactic studies were limited to Local Group galaxies. We are now able to obtain detailed inventories of sources in…

天体物理学 · 物理学 2007-05-23 Andrea H Prestwich

We have analyzed observations with the Chandra X-ray Observatory of the diffuse emission by hot gas in 7 dwarf starburst galaxies, 6 edge-on starburst galaxies, and 9 Ultra Luminous Infrared Galaxies. These systems cover ranges of \~ 10^4…

天体物理学 · 物理学 2009-11-10 J. P. Grimes , T. Heckman , D. Strickland , A. Ptak

Post-starburst galaxies are believed to be in a rapid transition between major merger starbursts and quiescent ellipticals, where AGN feedback is suggested as one of the processes responsible for the quenching. To study the role of AGN…

星系天体物理 · 物理学 2024-01-19 Dalya Baron , Hagai Netzer , Dieter Lutz , Ric I. Davies , J. Xavier Prochaska

We present here the first study of the X-ray properties of an evolutionary sample of merging galaxies. Both ROSAT PSPC and HRI data are presented for a sample of eight interacting galaxy systems, each believed to involve a similar encounter…

天体物理学 · 物理学 2009-10-30 A. M. Read , T. J. Ponman

This presentation reviews Chandra's major contribution to the understanding of nearby galaxies. After a brief summary on significant advances in characterizing various types of discrete X-ray sources, the presentation focuses on the global…

星系天体物理 · 物理学 2015-05-18 Q. Daniel Wang

Winds are predicted to be ubiquitous in low-mass, actively star-forming galaxies. Observationally, winds have been detected in relatively few local dwarf galaxies, with even fewer constraints placed on their timescales. Here, we compare…

星系天体物理 · 物理学 2018-04-11 Kristen B. W. McQuinn , Evan D. Skillman , Taryn N. Heliman , Noah P. Mitchell , Tyler Kelley

I discuss the empirical properties of diffuse X-ray emitting gas in the halos of both nearby starburst galaxies and normal spiral galaxies, based on high resolution X-ray spectral imaging with the Chandra X-ray Observatory. Diffuse thermal…

天体物理学 · 物理学 2007-05-23 David K. Strickland

The Chandra X-ray Observatory has completed a remarkable twenty years in orbit. A large part of the science program of Chandra during this time has involved the study of stars and their planetary systems. This primer aims to give the reader…

高能天体物理现象 · 物理学 2020-04-29 Jeremy J. Drake

We report on exploratory Chandra observations of five galactic nuclei that were found to be X-ray bright during the ROSAT all-sky survey (with L_X > 10^43 erg s^-1) but subsequently exhibited a dramatic decline in X-ray luminosity. Very…

天体物理学 · 物理学 2009-11-10 S. Vaughan , R. Edelson , R. S. Warwick

I provide an observational review of the properties of starburst-driven galactic superwinds, focusing mainly on recent results pertinent to the transport of metals and energy into the IGM. Absorption-line studies are providing rich…

天体物理学 · 物理学 2007-05-23 D. K. Strickland

In this paper we present the results of a 20 ks high resolution Chandra X-ray observation of the peculiar galaxy pair NGC 3395/3396, a system at a very early stage of merging, and less evolved than the famous Antennae and Mice merging…

天体物理学 · 物理学 2009-11-11 N. J. Brassington , A. M. Read , T. J. Ponman

Chandra is detecting a significant population of normal and starburst galaxies in extremely deep X-ray exposures. For example, approximately 15% of the sources arising in the 2 Ms Chandra Deep Field-North survey are fairly normal galaxies,…

Starburst galaxies are generally associated with extended X-ray and radio halos, giving a clear hint of an outflow of gas and relativistic particles from the disk into the halo. The driving agents are, not surprisingly, active star forming…

天体物理学 · 物理学 2007-05-23 Dieter Breitschwerdt

We report the results of an X-ray spectral imaging observation of the Antennae with the ROSAT PSPC. 55% of the soft X-ray flux from the system is resolved into discrete sources, including components identified with the galactic nuclei and…

天体物理学 · 物理学 2015-06-24 A. M. Read , T. J. Ponman , R. D. Wolstencroft

I review our recent Chandra surveys of the center region of the Milky Way and other nearby edge-on galaxies. Our Galactic center survey provides an unprecedented high-resolution, broad-band X-ray panorama of a 0.8x2 square degree swath…

天体物理学 · 物理学 2007-05-23 Q. Daniel Wang
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