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相关论文: Observations of Galaxies with Chandra

200 篇论文

A number of merging galaxy clusters shows the presence of shocks and cold fronts, i.e. sharp discontinuities in surface brightness and temperature. The observation of these features requires an X-ray telescope with high spatial resolution…

高能天体物理现象 · 物理学 2018-04-17 A. Botteon , F. Gastaldello , G. Brunetti

Over the past 16 years, NASA's Chandra X-ray Observatory has provided an unparalleled means for exploring the universe with its half-arcsecond angular resolution. Chandra studies have deepened our understanding of galaxy clusters, active…

天体物理仪器与方法 · 物理学 2015-05-06 Martin C. Weisskopf , Jessica Gaskin , Harvey Tananbaum , Alexey Vikhlinin

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

The Chandra X-ray Observatory is providing remarkable new views of massive star-forming regions, revealing all stages in the life cycle of high-mass stars and their effects on their surroundings. We present a Chandra tour of several…

天体物理学 · 物理学 2009-11-11 L. K. Townsley , P. S. Broos , E. D. Feigelson , G. P. Garmire

We present Chandra snapshot observations of the first large X-ray sample of optically identified fossil groups. For 9 of 14 candidate groups, we are able to determine the X-ray luminosity and temperature, which span a range typical of large…

宇宙学与河外天体物理 · 物理学 2009-10-23 Eric D. Miller , Eli Rykoff , Renato de Alencar Dupke , Claudia Mendes de Oliveira , Timothy McKay , Benjamin Koester

The presence of gaseous X-ray halos around massive galaxies is a basic prediction of all past and modern structure formation simulations. The importance of these X-ray halos is further emphasized by the fact that they retain signatures of…

星系天体物理 · 物理学 2023-04-05 Akos Bogdan , Mark Vogelsberger

A hot phase of the interstellar medium has now been detected and studied in several objects through its X-ray emission. A proper assessment of its characteristics is relevant for our understanding of several aspects of galaxy properties,…

天体物理学 · 物理学 2009-11-07 Ginevra Trinchieri

The past decade has seen a large progress in the X-ray investigation of early-type galaxies of the local universe, and first attempts have been made to reach redshifts z>0 for these objects, thanks to the high angular resolution and…

高能天体物理现象 · 物理学 2010-11-10 S. Pellegrini

We have performed uniform analysis of a sample of 54 nearby, early-type galaxies observed with \emph{Chandra}. In this work we present the spectral results for both the diffuse Interstellar Medium, ISM, and low-mass X-ray binaries, LMXBs.…

天体物理学 · 物理学 2007-11-06 Alex E Athey

The Chandra data archive after eight years' accumulation is a treasure for various studies, and in this paper we exploit this valuable resource to study the X-ray point source populations in nearby galaxies. By December 14, 2007, 383…

天体物理学 · 物理学 2011-03-04 Jifeng Liu

We review X-ray studies of the highest redshift (z > 4) quasars, focusing on recent advances enabled largely by the capabilities of Chandra and XMM-Newton. Included are discussions of basic X-ray population studies, X-ray spectroscopy,…

天体物理学 · 物理学 2007-05-23 W. N. Brandt , C. Vignali , X. Fan , S. Kaspi , D. P. Schneider

The Chandra Deep Fields (CDFs), being a major thrust among extragalactic X-ray surveys and complemented effectively by multiwavelength observations, have critically contributed to our dramatically improved characterization of the 0.5-8 keV…

星系天体物理 · 物理学 2017-09-26 Y. Q. Xue

I review Chandra's achievements in the last two years in AGN research. I concentrate on some topics of my interest; some others are reviewed in an accompanying article by K. Nandra. I comment briefly on the need to allow for the discovery…

天体物理学 · 物理学 2007-05-23 Smita Mathur

While often the point sources in X-ray surveys are dominated by AGN, with the high sensitivity of modern X-ray telescopes such as Chandra and XMM-Newton normal/starburst galaxies are also being detected in large numbers. We have made use of…

天体物理学 · 物理学 2009-11-13 A. Ptak

This "pedagogical" review describes the key Chandra and XMM-Newton extragalactic surveys to date and details some of their implications for AGN physics and evolution. We additionally highlight two topics of current widespread interest: (1)…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , D. M. Alexander , F. E. Bauer , C. Vignali

Within 40 years of the detection of the first extrasolar X-ray source in 1962,NASA's Chandra X-ray Observatory has achieved an increase in sensitivity of 10 orders of magnitude, comparable to the gain in going from naked-eye observations to…

高能天体物理现象 · 物理学 2014-06-02 H Tananbaum , M C Weisskopf , W Tucker , B Wilkes , P Edmonds

I summarize what is know about the evolution of galaxies in clusters from the observational point of view presenting results at high (z~1), intermediate (z~0.5) and low (z~0) redshifts. I comment on the comparison between observations and…

天体物理学 · 物理学 2007-05-23 B. M. Poggianti

I review recent results for quasars and discuss how they are related to activity in galaxies. Topics included are studies of quasar host galaxies with HST; searches for quasars in the Hubble Deep Field; evolution of the quasar luminosity…

天体物理学 · 物理学 2007-05-23 Patrick S. Osmer

We review recent results from Chandra observations of the X-ray bright cores of clusters of galaxies. We discuss the detection of ``cold fronts'' and their implication for thermal conduction, the interaction of cooling flow and radio source…

天体物理学 · 物理学 2007-05-23 S. Ettori , A. C. Fabian

The $Chandra$ archival data is a valuable resource for various studies on different topics of X-ray astronomy. In this paper, we utilize this wealth and present a uniformly processed data set, which can be used to address a wide range of…

太阳与恒星天体物理 · 物理学 2016-06-22 Song Wang , Jifeng Liu , Yanli Qiu , Yu Bai , Huiqin Yang , Jincheng Guo , Peng Zhang