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相关论文: ESO 381-47, an early-type galaxy with extended HI …

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ESO 243-49 is a high-mass (circular velocity $v_{\rm c}\approx200\,{\rm km\,s^{-1}}$) edge-on S0 galaxy in the Abell 2877 cluster at a distance of $\sim95\,{\rm Mpc}$. To elucidate the origin of its thick disc, we use MUSE science…

星系天体物理 · 物理学 2016-09-27 S. Comerón , H. Salo , R. F. Peletier , J. Mentz

We present HST/WFPC2 broadband and ground-based Halpha images, H I 21-cm emission maps, and low-resolution optical spectra of the nearby galaxy ESO 1327-2041, which is located 38 arcsec (14 kpc in projection) west of the quasar PKS…

宇宙学与河外天体物理 · 物理学 2012-06-15 B. A. Keeney , J. T. Stocke , C. W. Danforth , C. L. Carilli

We present a photometric study of UGC 4599, a low-luminosity galaxy superficially resembling Hoag's Object in that on sky survey images it appears to be a complete ring surrounding a roundish core. The nature of the outer ring of Hoag-type…

宇宙学与河外天体物理 · 物理学 2015-05-27 Ido Finkelman , Noah Brosch

The extreme outer Galaxy (EOG) has a very different environment from that in the solar neighborhood, with low metallicity (less than -0.5 dex), much lower gas density, and small or no perturbation from spiral arms. The EOG is an excellent…

天体物理学 · 物理学 2008-01-03 Naoto Kobayashi , Chikako Yasui , Alan T. Tokunaga , Masao Saito

We present the discovery of a 70 kpc X-ray tail behind the small late-type galaxy ESO137-001 in the nearby, hot (T=6.5 keV) merging cluster A3627, from both Chandra and XMM observations. The tail has a length-to-width ratio of ~ 10. It is…

天体物理学 · 物理学 2009-11-11 M. Sun , C. Jones , W. Forman , P. E. J. Nulsen , M. Donahue , M. Voit

We have discovered strong gravitational lensing by the galaxy ESO325-G004, in images obtained with the Advanced Camera for Surveys on the Hubble Space Telescope. The lens galaxy is a boxy group-dominant elliptical at z=0.0345, making this…

天体物理学 · 物理学 2009-11-11 Russell J. Smith , John P. Blakeslee , John R. Lucey , John Tonry

We present deep Halpha images of three nearby late-type spiral galaxies (NGC628, NGC1058 and NGC6946), which reveal the presence of HII regions out to, and beyond, two optical radii (defined by the 25th B-band isophote). The outermost HII…

天体物理学 · 物理学 2009-10-30 Annette Ferguson , Rosemary Wyse , Jay Gallagher , Deidre Hunter

We present a UV study of 3 extended UV (XUV) galaxies that we have observed with the UVIT and the GMRT. XUV galaxies show filamentary or diffuse star formation well beyond their optical disks, in regions where the disk surface density lies…

星系天体物理 · 物理学 2021-08-11 M. Das , Yadav , J. , Patra , N. , Dwarakanath , K. S. , McGaugh , S. S. , Schombert , J. , Rahna , P. T. , Murthy , J

We present deep BVRI band images and HI line observations of the nearby, low surface brightness galaxy ESO215-G?009 which were obtained with the ANU 2.3-m Telescope and the Australia Telescope Compact Array, respectively. ESO215-G?009 was…

天体物理学 · 物理学 2009-11-10 Bradley E. Warren , Helmut Jerjen , Baerbel S. Koribalski

Ram pressure stripping of the spiral galaxy ESO 137-001 within the highly dynamical intracluster medium (ICM) of the Norma cluster lead to spectacular extraplanar CO, optical, H$\alpha$, UV, and X-ray emission. The Halpha and X-ray tails…

星系天体物理 · 物理学 2024-12-04 B. Vollmer , M. Sun , P. Jachym , M. Fossati , A. Boselli

The outer regions of galactic disks have received increased attention since ultraviolet observations with GALEX demonstrated that nearly 30% of galaxies have UV emission beyond their optical extents, indicating star formation activity.…

星系天体物理 · 物理学 2015-05-18 Stephanie J. Bush , T. J. Cox , Christopher C. Hayward , David Thilker , Lars Hernquist , Gurtina Besla

We present a study of the physical properties of the disc and tail of ESO137-001, a galaxy suffering from extreme ram-pressure stripping during its infall into the Norma cluster. With sensitive and spatially-resolved MUSE spectroscopy, we…

星系天体物理 · 物理学 2016-01-22 Matteo Fossati , Michele Fumagalli , Alessandro Boselli , Giuseppe Gavazzi , Ming Sun , David J. Wilman

Though S0 galaxies are usually thought to be `red and dead', they often demonstrate weak star formation organised in ring structures and located in their outer disks. We try to clarify the nature of this phenomenon and its difference from…

星系天体物理 · 物理学 2023-01-18 O. Sil'chenko , A. Moiseev , D. Oparin , J. E. Beckman , J. Font

Observations of the rest-frame UV emission of high-redshift galaxies suggest that the early stages of galaxy formation involve disturbed structures. Imaging the cold interstellar medium can provide a unique view of the kinematics associated…

We study the properties of HI gas in the outer regions (~2r_25) of a spiral galaxy, UGC 00439 (z = 0.01769), using HI 21-cm absorption towards different components of an extended background radio source, J0041$-$0043 (z = 1.679). The radio…

星系天体物理 · 物理学 2016-01-20 Rajeshwari Dutta , Neeraj Gupta , Raghunathan Srianand , John O'Meara

We have mapped NGC 3718, a nearby bright galaxy in a loose group, and its companion NGC 3729 in the 21cm line of neutral hydrogen. NGC 3718 is a strikingly unusual galaxy with a strong straight dust lane across the center, peculiar diffuse…

星系天体物理 · 物理学 2009-11-13 Linda S. Sparke , Gustaaf van Moorsel , Ulrich J. Schwarz , Martin Vogelaar

Recent HI observations reveal that the discs of spiral galaxies are surrounded by extended gaseous haloes. This extra-planar gas reaches large distances (several kpc) from the disc and shows peculiar kinematics (low rotation and inflow). We…

天体物理学 · 物理学 2009-11-13 Filippo Fraternali , James Binney

A study is presented of HI line observations of the nearby spiral galaxy NGC 3521 observed with the VLA as part of The HI Nearby Galaxy Survey. Clearly evident in the HI data cube is the presence of an anomalous HI component that is both…

星系天体物理 · 物理学 2013-12-10 Edward Elson

We have observed the late-type peculiar galaxy NGC 4424 during VESTIGE, a blind narrow-band Halpha[NII] imaging survey of the Virgo cluster carried out with MegaCam at the CFHT. The presence of a 110 kpc long HI tail in the S direction…