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相关论文: NGC 5195 in M51: Feedback `Burps' after a Massive …

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We studied the nearby, interacting galaxy NGC 5195 (M51b) in the radio, optical and X-ray bands. We mapped the extended, low-surface-brightness features of its radio-continuum emission; determined the energy content of its complex structure…

We describe results from our initial study of the diffuse X-ray emission structures in NGC 5128 (Cen A) using the Chandra X-ray Observatory observations. The high-angular resolution Chandra images reveal multi-scale X-ray struct ures with…

天体物理学 · 物理学 2009-11-07 M. Karovska , G. Fabbiano , F. Nicastro , M. Elvis , R. P. Kraft , S. S. Murray

The early-type galaxy NGC 5195 (alternatively known as M51b) possesses extended gas features detected in multi-wavelength, postulated to be associated with previous activities of the central supermassive black hole (SMBH). Using integral…

星系天体物理 · 物理学 2023-02-01 Xiaoyu Xu , Junfeng Wang

High resolution OVRO CO 1-0 observations of the inner kpc of the M51-companion NGC 5195 reveal the presence of a kpc-sized bar, or possibly an inclined disk with a two armed spiral, at the center of the optical bar. The molecular mass of…

天体物理学 · 物理学 2007-05-23 S. Aalto , G. Rydbeck

The Whirlpool Galaxy is a well studied grand design galaxy with two major spiral arms, and a large satellite NGC 5195. The arms both show long uniform sections with perturbations ('kinks' or sharp turns) in specific regions. Comparing the…

星系天体物理 · 物理学 2025-02-24 Joan Font , John E. Beckman , Benoît Epinat , Clare L. Dobbs , Miguel Querejeta

We report on the imaging analysis of 200 ks sub-arcsecond resolution Chandra ACIS-S observations of the nearby Seyfert 1 galaxy NGC 4151. Bright, structured soft X-ray emission is observed to extend from 30 pc to 1.3 kpc in the south-west…

We present observations of the nearby barred starburst galaxy, M83 (NGC5236), with the new Fabry-Perot interferometer GHAFAS mounted on the 4.2 meter William Herschel Telescope on La Palma. The unprecedented high resolution observations, of…

We present a detailed imaging analysis of 260 ks of sub-arcsecond resolution Chandra Advanced CCD Imaging Spectrometer (ACIS-S) observations of the nearby Seyfert 2 galaxy NGC 5728. Our study focuses on the bright and diffuse soft X-ray…

星系天体物理 · 物理学 2024-11-01 Anna Trindade Falcao , G. Fabbiano , M. Elvis , A. Paggi , W. P. Maksym

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 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

Seyfert galaxy NGC 5252 harbors enormously extended ionization cones, which have been previously detected in the optical and X-ray band, offering a unique opportunity to investigate the interaction between the central active galactic…

高能天体物理现象 · 物理学 2024-01-18 Chen Wang , Junfeng Wang , Mauro Dadina , Giuseppina Fabbiano , Martin Elvis , Stefano Bianchi , Matteo Guainazzi

We report sub arc-second resolution X-ray imaging-spectroscopy of the archetypal type 2 Seyfert galaxy NGC 1068 with the Chandra X-ray Observatory. The observations reveal the detailed structure and spectra of the 13 kpc-extent nebulosity…

天体物理学 · 物理学 2009-11-06 A. J. Young , A. S. Wilson , P. L. Shopbell

M51 and NGC 5195 is an interacting system that can be explored in great details with ground-based telescopes. The H II regions in M51 were observed using the 2.16 m telescope of the National Astronomical Observatories of the Chinese Academy…

星系天体物理 · 物理学 2020-08-19 Peng Wei , Hu Zou , Xu Kong , Xu Zhou , Ning Hu , Zesen Lin , Yewei Mao , Lin Lin , Zhimin Zhou , Xiang Liu , Shuguo Ma , Lu Ma , Tuhong Zhong , Fei Dang , Jiantao Sun , Xinkui Lin

An extended component of X-ray emission has been detected in Seyfert galaxies - NGC 1365 and NGC 4051, using the ROSAT HRI. Its size is about 2 kpc and it contains 56% +- 8% of the total observed flux in NGC 1365, and 21% +- 6% in NGC 4051.…

天体物理学 · 物理学 2009-09-25 Kulinder Pal Singh

High-spatial resolution near-infrared (NIR) images of the central 24 x 24 arcsec^2 (~ 2 x 2 kpc^2) of the elliptical galaxy NGC 1052 reveal a total of 25 compact sources randomly distributed in the region. Fifteen of them exhibit Halpha…

宇宙学与河外天体物理 · 物理学 2015-05-20 J. A. Fernández-Ontiveros , C. López-Sanjuan , M. Montes , M. A. Prieto , J. A. Acosta-Pulido

The M51 galaxy is one of best examples of grand design structure in galaxies. The most likely origin of the spiral arms in M51 is the ongoing interaction with NGC 5195. Here we report recent calculations which model the orbit of M51 and NGC…

星系天体物理 · 物理学 2009-08-26 C. L. Dobbs , C. Theis , J. E. Pringle , M. R. Bate

We report the analysis of deep radio observations of the interacting galaxy system M51 from the Very Large Array, with the goal of understanding the nature of the population of compact radio sources in nearby spiral galaxies. We detect 107…

天体物理学 · 物理学 2008-11-26 L. A. Maddox , J. J. Cowan , R. E. Kilgard , E. Schinnerer , C. J. Stockdale

New observations using narrow band imaging, long-slit spectroscopy and MERLIN observations of the nuclear region of the Seyfert galaxy NGC~4051 have been made. An edge brightened, triangular region of ionized gas extending 420 pc from the…

We report on Atacama Large Millimeter Array (ALMA) observations of CO(3-2) emission in the Seyfert2/starburst galaxy NGC1808, at a spatial resolution of 4pc. Our aim is to investigate the morphology and dynamics of the gas inside the…

We present moderately-high resolution echelle observations of the nucleus of NGC 5195, the line of sight to which samples intervening interstellar material associated with the outer spiral arm of M51. Our spectra reveal absorption from…

星系天体物理 · 物理学 2018-06-07 Adam M. Ritchey , George Wallerstein
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