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We present the results of a targeted search for intervening HI absorption in six nearby, gas-rich galaxies using the Australia Telescope Compact Array (ATCA). The sightlines searched have impact parameters of 10-20 kpc. By targeting nearby…

星系天体物理 · 物理学 2015-06-24 S. N. Reeves , E. M. Sadler , J. R. Allison , B. S. Koribalski , S. J. Curran , M. B. Pracy

We theoretically study the vertical structure of the edge-on low surface brightness (LSB) galaxy UGC 7321. This is one of the few well-observed LSBs. We modeled it as a gravitationally coupled disk system of stars and atomic hydrogen gas in…

星系天体物理 · 物理学 2019-08-30 Suchira Sarkar , Chanda J. Jog

The dominant physical processes responsible for the formation and longevity of giant gaseous and stellar discs in galaxies remain controversial. Although they are rare (less than 10 confirmed as of now), giant low-surface brightness (gLSB)…

星系天体物理 · 物理学 2019-09-25 Anna Saburova , Igor Chilingarian , Anastasia Kasparova , Ivan Katkov , Daniel Fabricant , Roman Uklein

We built a multi-wavelength dataset for galaxies from the Local Volume HI Survey (LVHIS), which comprises 82 galaxies. We also select a sub-sample of ten large galaxies for investigating properties in the galactic outskirts. The LVHIS…

Giant low-surface brightness (GLSB) galaxies are an extreme class of objects with very faint and extended gas-rich disks. Malin 1 is the largest GLSB galaxy known to date, but its formation is still poorly understood. We use VLT/MUSE IFU…

星系天体物理 · 物理学 2024-01-24 Junais , P. M. Weilbacher , B. Epinat , S. Boissier , G. Galaz , E. J. Johnston , T. H. Puzia , P. Amram , K. Małek

Five galaxy groups with properties similar to those of the Local Group have been surveyed for HI clouds with the Arecibo Telescope. In total 300 pointings have been observed on grids of approximately 2.5 x 1.5 Mpc centred on the groups. The…

天体物理学 · 物理学 2009-11-06 Martin Zwaan

A total of 367 Low Surface Brightness galaxies detected in the 2MASS all-sky near-infrared survey have been observed in the 21 cm HI line using the Arecibo telescope. All have a K_s-band mean central surface brightness, measured within a 5…

天体物理学 · 物理学 2009-11-07 D. Monnier Ragaigne , W. van Driel , K. O'Neil , S. E. Schneider , C. Balkowski , T. H. Jarrett

Giant low-surface-brightness disk galaxies (gLSBGs) are rare objects with disk radii up-to 160 kpc and dynamical masses of an order of up to 10$^{12}$ $M_{\odot}$. Their very existence challenges currently accepted theories of galaxy…

The nearby galaxy HIZSS003 was recently discovered during a blind HI survey of the zone of avoidance (Henning et al. 2000). Follow up VLA as well as optical and near-IR imaging and spectroscopy (Massey et al. 2003; Silva et al. 2005)…

天体物理学 · 物理学 2009-11-10 Ayesha Begum , Jayaram N. Chengalur , I. D. Karachentsev , M. E. Sharina

Giant low surface brightness (GLSB) galaxies are commonly thought to be massive, dark matter dominated systems. However, this conclusion is based on highly uncertain rotation curves. We present here a new study of two prototypical GLSB…

宇宙学与河外天体物理 · 物理学 2015-05-18 Federico Lelli , Filippo Fraternali , Renzo Sancisi

We present the analysis of the diffuse, low column density HI environment of 18 MHONGOOSE galaxies. We obtained deep observations with the Robert C. Byrd Green Bank Telescope, and reached down to a 3sigma column density detection limit of…

星系天体物理 · 物理学 2021-04-07 Amy Sardone , D. J. Pisano , N. M. Pingel , Amidou Sorgho , Claude Carignan , W. J. G. de Blok

HI features near young star clusters in M81 are identified as the photodissociated surfaces of Giant Molecular Clouds (GMCs) from which the young stars have recently formed. The HI column densities of these features show a weak trend, from…

天体物理学 · 物理学 2008-11-26 Jonathan S. Heiner , Ronald J. Allen , Bjorn H. C. Emonts , Pieter C. van der Kruit

We present 46 rest-frame ultraviolet (UV) spectra of 28 local starburst and star-forming galaxies which were observed with the Faint Object Spectrograph (FOS) and the Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope…

宇宙学与河外天体物理 · 物理学 2015-05-20 Claus Leitherer , Christy A. Tremonti , Timothy M. Heckman , Daniela Calzetti

We present results from 21 cm radio synthesis imaging of 28 spiral galaxies from the DiskMass Survey obtained with the VLA, WSRT, and GMRT facilities. We detail the observations and data reduction procedures and present a brief analysis of…

We present the results of HI observations of five groups of galaxies spanning a range of velocity dispersion and spiral fraction (brightest optical group member in parenthesis): NGC 7582 (NGC 7552), USGC U207 (NGC 2759), USGC U070 (NGC…

宇宙学与河外天体物理 · 物理学 2015-05-13 E. Freeland , A. Stilp , E. Wilcots

HI observations of the nearby blue compact dwarf galaxy IC 10 obtained with the Dominion Radio Astrophysical Observatory synthesis telescope (DRAO), for a total integration of $\sim$1000 hours, are presented. We confirm the NW faint 21 cm…

星系天体物理 · 物理学 2020-01-08 Brenda Namumba , Claude Carignan , Tyler Foster , Nathan Deg

We present a deep Giant Metrewave Radio Telescope (GMRT) search for HI 21 cm emission from three dwarf galaxies, viz. POX 186, SC 24 and KKR 25. Based, in part, on previous single dish HI observations, these galaxies have been classified as…

天体物理学 · 物理学 2009-11-13 Ayesha Begum , Jayaram N. Chengalur

Superthin galaxies (STs) are edge-on disc galaxies with strikingly high planar-to-vertical axes ratios of $\sim 10 - 20$ with no bulge component, and central surface brightness in $B$-band $>$ 23 mag arcsec$^{-2}$ comparable to low surface…

星系天体物理 · 物理学 2022-06-22 Ganesh Narayanan , Arunima Banerjee

Very sensitive HI 21cm observations have been made in 860 directions at dec >= -43deg in search of weak, Galactic, high-velocity HI emission lines at moderate and high Galactic latitudes. One-third of the observations were made toward…

天体物理学 · 物理学 2009-11-07 Felix J. Lockman , Edward M. Murphy , Sara Petty-Powell , Vincent J. Urick

Giant low surface brightness galaxies (GLSBs), such as Malin 1, have unusually large and flat discs. Their formation is a puzzle for cosmological simulations in the cold dark matter scenario. We suggest that GLSBs might be the final product…

宇宙学与河外天体物理 · 物理学 2009-02-23 M. Mapelli , B. Moore