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相关论文: Dynamics of Starbursting Dwarf Galaxies. III. A HI…

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Strong bursts of star formation in galaxies may be triggered either by internal or external mechanisms. We study the distribution and kinematics of the HI gas in the outer regions of 18 nearby starburst dwarf galaxies, that have accurate…

星系天体物理 · 物理学 2015-06-22 Federico Lelli , Marc Verheijen , Filippo Fraternali

VLA and Parkes 64 m radiotelescope 21-cm observations of the starburst dwarf galaxy NGC 5253 reveal a multi-component non-axisymmetric HI distribution. The component associated with the stellar body shows evidence for a small amount of…

天体物理学 · 物理学 2009-11-13 Henry A. Kobulnicky , Evan. D. Skillman

We present a method to derive the dynamical mass of face-on galaxy disks using their neutral hydrogen (HI) velocity dispersion. We have applied the method to nearby, gas rich galaxies that have extended HI gas disks and have low…

星系天体物理 · 物理学 2020-02-05 Mousumi Das , Stacy McGaugh , Roger Ianjamasimanana , James Schombert , K. S. Dwarakanath

UGC 4483 is a nearby Blue Compact Dwarf (BCD) galaxy. HST observations have resolved the galaxy into single stars and this has led to the derivation of its star formation history and to a direct estimate of its stellar mass. We have…

宇宙学与河外天体物理 · 物理学 2015-06-05 Federico Lelli , Marc Verheijen , Filippo Fraternali , Renzo Sancisi

I Zw 18 is a prototype Blue Compact Dwarf (BCD), characterized by a strong starburst and extremely low metallicity (Z ~ 0.02 Zsun). It has long been considered a candidate young galaxy in the Local Universe, but recent studies indicate the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Federico Lelli , Marc Verheijen , Filippo Fraternali , Renzo Sancisi

We study the gas kinematics of a sample of six isolated gas-rich low surface brightness galaxies, of the class called ultra-diffuse galaxies (UDGs). These galaxies have recently been shown to be outliers from the baryonic Tully-Fisher…

Dwarf Irregular galaxies (dIrrs) are the smallest stellar systems with extended HI discs. The study of the kinematics of such discs is a powerful tool to estimate the total matter distribution at these very small scales. In this work, we…

To explore the properties of extreme outer stellar disks, we obtained ultra-deep V and GALEX UV images of 4 dwarf irregular galaxies and one Blue Compact Dwarf galaxy and ultra-deep B images of 3 of these. Our V-band surface photometry…

宇宙学与河外天体物理 · 物理学 2015-05-28 Deidre A. Hunter , Bruce G. Elmegreen , Se-Heon Oh , Ed Anderson , Tyler E. Nordgren , Philip Massey , Nick Wilsey , Malanka Riabokin

Gas velocity dispersions provide important diagnostics of the forces counteracting gravity to prevent collapse of the gas. We use the 21 cm line of neutral atomic hydrogen (HI) to study HI velocity dispersion and HI phases as a function of…

We have studied multi-band surface brightness profiles of a representative sample of 34 nearby dwarf irregular galaxies (dIrrs). Our data include GALEX FUV/NUV, UBV, H\alpha, and Spitzer 3.6 \mum images. These galaxies constitute the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Hong-Xin Zhang , Deidre A. Hunter , Bruce G. Elmegreen , Yu Gao , Andreas Schruba

We have examined gas engaged in noncircular motions in 22 of the nearby LITTLE THINGS dwarf irregular galaxies. The HI data cubes have been deconvolved into kinematic components - bulk rotation and noncircular motions, to produce maps of…

星系天体物理 · 物理学 2019-06-26 Deidre A. Hunter , Lauren Laufman , Se-Heon Oh , Stephen E. Levine , Caroline E. Simpson

We identify some of the most HI massive and fastest rotating disk galaxies in the local universe with the aim of probing the processes that drive the formation of these extreme disk galaxies. By combining data from the Cosmic Flows project,…

星系天体物理 · 物理学 2015-06-23 H. M. Courtois , D. Zaritsky , J. G. Sorce , D. Pomarede

The radial profiles of gas, stars, and far ultraviolet radiation in 20 dwarf Irregular galaxies are converted to stability parameters and scale heights for a test of the importance of two-dimensional (2D) instabilities in promoting star…

星系天体物理 · 物理学 2015-06-03 Bruce G. Elmegreen , Deidre A. Hunter

Recent studies have shown that starburst dwarf galaxies have steeply rising rotation curves in their inner parts, pointing to a close link between the intense star formation and a centrally concentrated mass distribution (baryons and dark…

We identify 814 discrete HI clouds in 40 dwarf irregular galaxies from the LITTLE THINGS survey using an automated cloud-finding algorithm. The cloud masses range from ~10^3 to 10^7 Msolar, have a surface density averaged over all of the…

星系天体物理 · 物理学 2019-06-05 Deidre A. Hunter , Bruce G. Elmegreen , Clara L. Berger

We present WSRT observations of high sensitivity and resolution of the neutral hydrogen in the starburst dwarf galaxy NGC 1569. Assuming a distance of 2.2 Mpc, we find a total HI mass of 1.3 * 10^8 M_sun to be distributed in the form of a…

天体物理学 · 物理学 2009-11-07 J. M. Stil , F. P. Israel

We present ionized gas kinematics for 681 galaxies at $z\sim 1.4-3.8$ from the MOSFIRE Deep Evolution Field survey, measured using models which account for random galaxy-slit misalignments together with structural parameters derived from…

We present new multi-configuration HI aperture synthesis imaging of the nearby dwarf starburst galaxy NGC 625 obtained with the Australia Telescope Compact Array. Total HI column density images show gas well-aligned with the optical major…

天体物理学 · 物理学 2009-11-10 John M. Cannon , N. M. McClure-Griffiths , Evan D. Skillman , Stephanie Cote

We report the discovery of a rare isolated group of five dwarf galaxies located at z = 0.0086 ($D$ = 36 Mpc). All member galaxies are star-forming, blue, and gas-rich with $g-r$ indices ranging from 0.2 to 0.6 mag, and two of them show…

星系天体物理 · 物理学 2024-11-18 Sanjaya Paudel , Cristiano G. Sabiu , Suk-Jin Yoon , Pierre-Alain Duc , Jaewon Yoo , Oliver Müller

We present resolved HI observations of six dwarf galaxies drawn from a sample of baryon-dominated dwarf galaxy (BDDG) candidates previously identified using global HI spectra from ALFALFA and optical inclinations from SDSS, both of which…

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