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相关论文: CHANG-ES XXIX: The Sub-kpc Nuclear Bubble of NGC 4…

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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

We present near-infrared VLT ISAAC imaging and spectroscopy of the peculiar Virgo galaxy NGC 4438, whose nucleus has been classified as a LINER. The data are supplemented by mid-infrared imaging, and compared to previous WFPC2 HST broadband…

星系天体物理 · 物理学 2015-05-14 Sebastian Perez , Simon Casassus , Juan R. Cortes , J. D. P. Kenney

We present Chandra ACIS-I and ACIS-S observations (~200ks in total) of the X-ray luminous elliptical galaxy NGC4636, located in the outskirts of the Virgo cluster. A soft band (0.5-2 keV) image shows the presence of a bright core in the…

宇宙学与河外天体物理 · 物理学 2009-12-07 A. Baldi , W. Forman , C. Jones , R. Kraft , P. Nulsen , E. Churazov , L. David , S. Giacintucci

We present Chandra ACIS-I and ACIS-S observations ($\sim$200 ks in total) of the X-ray luminous elliptical galaxy NGC 4636, located in the outskirts of the Virgo cluster. A soft band (0.5-2 keV) image shows the presence of a bright core in…

宇宙学与河外天体物理 · 物理学 2015-05-14 A. Baldi , W. Forman , C. Jones , R. Kraft , P. Nulsen , E. Churazov , L. David , S. Giacintucci

We present broadband and narrowband Hubble Space Telescope images of the central region of the heavily disturbed Virgo cluster galaxy NGC 4438 (Arp120), whose nucleus has been described as a type 1 LINER or dwarf Seyfert. Narrowband H-alpha…

天体物理学 · 物理学 2007-05-23 Jeffrey D. P. Kenney , Elizabeth E. Yale

Superbubbles in the nuclear region of galaxies could be produced by the AGN or nuclear starburst via different driving forces. We report analysis of the multi-wavelength data of the kpc-scale nuclear superbubble in NGC 3079, in order to…

星系天体物理 · 物理学 2024-04-08 Jiang-Tao Li , Wei Sun , Li Ji , Yang Yang

The X-ray properties of 15 nearby (v<3,000 km/s) galaxies that possess AGN and/or starbursts are discussed. Two-thirds have nuclear extended emission on scales from ~0.5 to ~1.5 kpc that is either clearly associated with a nuclear outflow…

天体物理学 · 物理学 2007-05-23 Kimberly A. Weaver

We present the Chandra discovery of soft diffuse X-ray emission in NGC 4151 (L[0.5-2keV]~10^{39} erg s$^{-1}$), extending ~2 kpc from the active nucleus and filling in the cavity of the HI material. The best fit to the X-ray spectrum…

We present evidence of the co-existence of either an AGN or an ultraluminous X-ray source (ULX), together with a young super stellar cluster in the 3 central parsecs of NGC4303. The galaxy contains a low luminosity AGN and hosts a number of…

The analysis of a deep (579 ks) Chandra ACIS pointing of the elliptical galaxy NGC4278, which hosts a low luminosity AGN and compact radio emission, allowed us to detect extended emission from hot gas out to a radius of \sim 5 kpc, with a…

高能天体物理现象 · 物理学 2015-06-05 S. Pellegrini , J. Wang , G. Fabbiano , D. W. Kim , N. J. Brassington , J. S. Gallagher , G. Trinchieri , A. Zezas

Observations made during the last ten years with the Chandra X-ray Observatory have shed much light on the cooling gas in the centers of clusters of galaxies and the role of active galactic nucleus (AGN) heating. Cooling of the hot…

宇宙学与河外天体物理 · 物理学 2019-08-14 Elizabeth L. Blanton , T. E. Clarke , Craig L. Sarazin , Scott W. Randall , Brian R. McNamara

The evolution of Active Galactic Nuclei (AGN) is closely connected to their host galaxies and surroundings. Via feedback processes, AGN can counteract the cooling of the intracluster medium (ICM) and suppress star formation in their host…

高能天体物理现象 · 物理学 2024-10-16 A. Spasic , H. W. Edler , Y. Su , M. Brüggen , F. de Gasperin , T. Pasini , V. Heesen , M. Simonte , A. Boselli , H. J. A. Röttgering , M. Fossati

We present {\it Gemini} longslit optical spectroscopy and VLA radio observations of the nuclear region of NGC 4178, a late-type bulgeless disk galaxy recently confirmed to host an AGN through infrared and X-ray observations. Our…

宇宙学与河外天体物理 · 物理学 2015-06-17 Nathan Secrest , Shobita Satyapal , Sean Moran , Teddy Cheung , Marcello Giroletti , Mario Gliozzi , Marcel Bergmann , Anil Seth

The hot plasma permeating clusters of galaxies often shows a central peak in the X-ray surface brightness that is coincident with a drop in entropy. This is taken as evidence for a cooling flow where the radiative cooling in the central…

天体物理学 · 物理学 2015-06-24 Marcus Brueggen , Christian R. Kaiser

The aim of this study is to constrain the dynamics, structure and feeding of the compact nucleous of NGC4418, and to reveal the nature of the main hidden power source: starburst or AGN. We obtained high spatial resolution observations of…

星系天体物理 · 物理学 2015-06-16 F. Costagliola , S. Aalto , K. Sakamoto , S. Martín , R. Beswick , S. Muller , H. -R. Klöckner

We report the Chandra detection of X-ray emission spatially coincident with the kpc-scale radio bubbles in the nearby (D_L ~ 31 Mpc) AGN-starburst galaxy NGC 6764. The X-ray emission originates in hot gas (kT ~ 0.75 keV), which may either…

天体物理学 · 物理学 2009-11-13 J. H. Croston , M. J. Hardcastle , P. Kharb , R. P. Kraft , A. Hota

Seyfert-starburst composite galaxies host two promising phenomena of non-thermal high-energy radiation. In this regard the IceCube observation of high-energy neutrinos from the direction of the Seyfert-starburst composite galaxy NGC 1068 is…

高能天体物理现象 · 物理学 2025-09-23 Silvia Salvatore , Björn Eichmann , Giacomo Sommani , Santiago del Palacio , Patrik M. Veres , Julia Becker Tjus

Observations of the Seyfert 2 and starburst galaxy NGC 5135 with the Chandra X-ray Observatory demonstrate that both of these phenomena contribute significantly to its X-ray emission. We spatially isolate the active galactic nucleus (AGN)…

天体物理学 · 物理学 2016-08-30 N. A. Levenson , K. A. Weaver , T. M. Heckman , H. Awaki , Y. Terashima

The presence of multi-phase outflows in low ionisation nuclear emission-line regions (LINERs) has been confirmed to be frequent, but the mechanisms that launch them are still under study. We aim to explore the connections between the…

NGC 4477 is a low-mass lenticular galaxy in the Virgo Cluster, residing at 100\,kpc to the north of M87. Using a total of 116\,ks {\sl Chandra} observations, we study the interplay between its hot ($\sim$0.3\,keV) gas halo and the central…

星系天体物理 · 物理学 2019-04-23 Yijia Li , Yuanyuan Su , Christine Jones
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