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By combining HST imaging with optical (VIMOS) and near-infrared (SINFONI) integral field spectroscopy we exploit the gravitational potential of a massive, rich cluster at z=0.9 to study the internal properties of a gravitationally lensed…

天体物理学 · 物理学 2008-11-26 A. M. Swinbank , R. G. Bower , G. P. Smith , R. J. Wilman , Ian Smail , R. S. Ellis , S. L. Morris , J. -P. Kneib , ;

New ALMA CO, HCO+, and 100 GHz continuum observations and Gemini NIFS K-band spectra are combined with previous radio to X-ray data to study Feature i, a highly luminous starburst clump on an outer arm of the interacting galaxy NGC 2207.…

We successfully detected a molecular outflow with a scale of 370-450 pc in the central region of the starburst galaxy NGC 3628 through deep CO(1-0) observations by using the Nobeyama Millimeter Array (NMA). The mass of the outflowing…

星系天体物理 · 物理学 2015-06-04 An-Li Tsai , Satoki Matsushita , Albert K. H. Kong , Hironori Matsumoto , Kotaro Kohno

Context: H\alpha images of star bursting irregular galaxies reveal a large amount of extended ionized gas structures, in some cases at kpc-distance away from any place of current star forming activity. A kinematic analysis of especially the…

天体物理学 · 物理学 2009-11-13 J. van Eymeren , D. J. Bomans , K. Weis , R. -J. Dettmar

We present the kinematics of the ionized gas over the inner 140 arcsec (10 kpc) of NGC 1068 from observations with the HIFI Fabry-Perot interferometer. There is clear evidence for density wave streaming and bar-driven streaming across the…

天体物理学 · 物理学 2011-03-10 W. Dehnen , J. Bland-Hawthorn , A. Quirrenbach , G. Cecil

We present an analysis of the molecular and atomic gas emission in the rest-frame far-infrared and sub-millimetre, from the lensed z=2.3 sub-millimetre galaxy SMM J2135-0102. We obtain very high signal-to-noise detections of 11 transitions…

We present the results of a near-infrared and X-ray study of the Seyfert 2 galaxy NGC 3281. Emission from the Seyfert nucleus is detected in both regions of the electromagnetic spectrum, allowing us to infer both the equivalent line of…

天体物理学 · 物理学 2009-10-30 Chris Simpson , Subaru Telescope

Actively accreting supermassive black holes significantly impact the evolution of their host galaxies, truncating further star formation by expelling large fractions of gas with wide-angle outflows. The X-ray band is key to understanding…

高能天体物理现象 · 物理学 2022-10-05 A. Ogorzalek , A. L. King , S. W. Allen , J. C. Raymond , D. R. Wilkins

The nearby dwarf galaxy II Zw 40 hosts an intense starburst. At the center of the starburst is a bright compact radio and infrared source, thought to be a giant dense HII region containing ~14,000 O stars. Radio continuum images suggest…

星系天体物理 · 物理学 2015-06-15 Sara Beck , Jean Turner , John Lacy , Thomas Greathouse , Ohr Lahad

We report the results of a study of the rest-frame UV spectrum of the Cosmic Eye, a luminous Lyman break galaxy at z=3.07331 gravitationally lensed by a factor of 25. The spectrum, recorded with the ESI spectrograph on the Keck II…

宇宙学与河外天体物理 · 物理学 2015-05-14 Anna M. Quider , Alice E. Shapley , Max Pettini , Charles C. Steidel , Daniel P. Stark

We found a very large, 35 kpc, emission-line region around the Seyfert type 2 galaxy NGC 4388, using deep narrow-band imaging with the prime focus camera (Suprime-Cam) of the Subaru telescope. This region consists of many faint gas clouds…

We present the analysis of the multi-phase gas properties in the Seyfert II galaxy NGC 424, using spatially resolved spectroscopic data from JWST/MIRI, part of the Mid-InfraRed Activity of Circumnuclear Line Emission (MIRACLE) program, as…

NGC 4945 is a Seyfert 2 galaxy at a distance of 3.82 Mpc. Its relative proximity has permitted a detailed SMA study of the circumnuclear molecular gas in a galaxy exhibiting an AGN. Based on an analysis of the high-resolution velocity field…

宇宙学与河外天体物理 · 物理学 2015-05-27 Lien-Hsuan Lin , Ronald E. Taam , David C. C. Yen , S. Muller , J. Lim

The nearby radio galaxy 3C293 is one of a small group of objects where extreme outflows of neutral hydrogen have been detected. However, due to the limited spatial resolution of previous observations, the exact location of the outflow was…

宇宙学与河外天体物理 · 物理学 2015-06-16 Elizabeth Mahony , Raffaella Morganti , Bjorn Emonts , Tom Oosterloo , Clive Tadhunter

We present the discovery of an outflowing ionized wind in the Seyfert 1 Galaxy Mrk 335. Despite having been extensively observed by most of the largest X-ray observatories in the last decade, this bright source was not known to host warm…

宇宙学与河外天体物理 · 物理学 2015-06-12 A. L. Longinotti , Y. Krongold , G. Kriss , J. Ely , L. Gallo , D. Grupe , S. Komossa , S. Mathur , A. Pradhan

We present a simple kinematic model for the narrow-line region (NLR) of the Seyfert 1 galaxy NGC 4151, based on our previous observations of extended [O III] emission with the Space Telescope Imaging Spectrograph (STIS). The model is…

We present the BeppoSAX broad-band X-ray spectrum of the Seyfert 2 galaxy NGC 3281. The source high-energy spectrum is characterized by the nuclear transmitted component, with an absorbing column density of about 2 10^24 cm^-2, while the…

天体物理学 · 物理学 2009-11-07 C. Vignali , A. Comastri

[Abridged] We present Gemini-N GMOS-IFU observations of the central starburst clumps and inner wind of M82, together with WIYN DensePak IFU observations of the inner 2x0.9kpc of the disk. These cover the emission lines of H$\alpha$, [NII],…

星系天体物理 · 物理学 2011-02-11 M. S. Westmoquette , L. J. Smith , J. S. Gallagher , G. Trancho , N. Bastian , I. S. Konstantopoulos

We report our Keck/MOSFIRE and Magellan/LDSS3 spectroscopy for an [OII] Blob, OIIB10, that is a high-$z$ galaxy with spatially extended [OII]$\lambda\lambda3726,3729$ emission over 30 kpc recently identified by a Subaru large-area…

星系天体物理 · 物理学 2015-06-22 Yuichi Harikane , Masami Ouchi , Suraphong Yuma , Michael Rauch , Kimihiko Nakajima , Yoshiaki Ono

The physical conditions in the inner narrow line region (NLR) of the Seyfert 2 galaxy, NGC 1068, are examined using ultraviolet and optical spectra and photoionization models. The spectra are Hubble Space Telescope (HST) Harchive data…

天体物理学 · 物理学 2009-10-30 Steven B. Kraemer , Jose R. Ruiz , D. Michael Crenshaw
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