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相关论文: The Local Environment of HII Galaxies

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We have carried out an investigation of the environments of low redshift HII galaxies by cross-correlating their positions on the sky with those of faint field galaxies in the Automatic Plate Measuring Machine catalogues. We address the…

天体物理学 · 物理学 2009-10-31 Eduardo Telles , Steve Maddox

Recent morphological studies (Telles \& Terlevich 1994) of HII galaxies, i.e. dwarf galaxies dominated by a very luminous starburst, have indicated that luminous HII galaxies tend to show distorted morphology suggestive of tidal…

天体物理学 · 物理学 2015-06-24 Eduardo Telles , Roberto Terlevich

I study the VLA HI survey of HII galaxies by Taylor et al. (1995, ApJS, 99, 427; 1996, ApJS, 102, 189) and the VLA HI survey of low surface brightness (LSB) dwarf galaxies by Taylor et al. (1996, ApJS, in press) to investigate the role of…

天体物理学 · 物理学 2009-10-28 Christopher L. Taylor

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

A sample of 69 galaxies with radial velocities less than 2500 km/s was selected from the HI Parkes All Sky Survey (HIPASS) to deduce details about star formation in nearby disk galaxies selected with no bias to optical surface brightness…

天体物理学 · 物理学 2009-11-11 J. F. Helmboldt , R. A. M. Walterbos , G. D. Bothun , K. O'Neil

We present a study of the close (< 200 kpc) environment of 110 relatively local (z< 0.16) HII galaxies, selected from the Sloan Digital Sky Survey (SDSS; DR7). We use available spectroscopic and photometric redshifts in order to investigate…

宇宙学与河外天体物理 · 物理学 2014-07-17 E. Koulouridis , M. Plionis , R. Chávez , E. Terlevich , R. Terlevich , F. Bresolin , S. Basilakos

We have discovered a number of very small isolated HII regions 20-30 kpc from their nearest galaxy. The HII regions appear as tiny emission line dots (ELdots) in narrow band images obtained by the NOAO Survey for Ionization in Neutral Gas…

天体物理学 · 物理学 2007-05-23 E. V. Ryan-Weber , M. E. Putman , K. C. Freeman , G. R. Meurer , R. L. Webster

A number of very small isolated HII regions have been discovered at projected distances up to 30 kpc from their nearest galaxy. These HII regions appear as tiny emission line objects in narrow band images obtained by the NOAO Survey for…

天体物理学 · 物理学 2015-06-24 E. V. Ryan-Weber , G. R. Meurer , K. C. Freeman , M. E. Putman , R. L. Webster , the SINGG team

Observations show that galaxies in galaxy clusters are strongly influenced by their environment. There is growing evidence that some galaxies in groups show similar properties to galaxies in clusters, such as redder colours and gas…

星系天体物理 · 物理学 2014-06-19 Helga Dénes , Virginia A. Kilborn , Bärbel S. Koribalski

In this paper, we present some correlations of neutral hydrogen HI gas and physical properties of galaxies to investigate the role of atomic gas in governing galaxy evolution. We build a HI-detected sample including 70 galaxies that are…

星系天体物理 · 物理学 2018-08-08 Zhimin Zhou , Hong Wu , Xu Zhou , Jun Ma

High spatial and spectral resolution observations of the atomic interstellar medium in nearby dwarf galaxies reveal evidence for warm and cold neutral gas, just like the phases in our own Galaxy. The cold or quiescent phase (about 20% of…

天体物理学 · 物理学 2009-04-13 L. M. Young , L. van Zee , R. C. Dohm-Palmer , K. Y. Lo

We have searched for companion galaxies in the close environment of 98 star-forming dwarf galaxies (SFDGs) from field and low density environments, using the NASA Extragalactic Database. Most of the companions are dwarf galaxies which due…

天体物理学 · 物理学 2009-11-06 K. G. Noeske , J. Iglesias-Paramo , J. M. Vilchez , P. Papaderos , K. J. Fricke

We have investigated how the incidence of star-forming galaxies varies with the environment using a volume-limited sample of nearby galaxy spectra extracted from the 2dF Galaxy Redshift Survey. The environment is characterized by the local…

天体物理学 · 物理学 2007-05-23 Laerte Sodre , Abilio Mateus

We use HI data from the FAST Extended Atlas of Selected Targets Survey (FEASTS) to study the interplay between gas and star formation of galaxies in interacting systems. We build control and mock HI disks and parameterize HI disorder by a…

星系天体物理 · 物理学 2025-02-13 Shun Wang , Jing Wang , Karen Lee-Waddell , Dong Yang , Xuchen Lin , Lister Staveley-Smith

The Local Group hosts a number of star-forming dwarf galaxies that show evidence of periods of little to no star formation. We use a suite of cosmological simulations to study how star formation is reignited in such galaxies. We focus on…

星系天体物理 · 物理学 2018-10-15 Anna C. Wright , Alyson M. Brooks , Daniel R. Weisz , Charlotte R. Christensen

We have explored the role environmental factors play in determining characteristics of young stellar objects in nearby dwarf irregular and Blue Compact Dwarf galaxies. Star clusters are characterized by concentrations, masses, and formation…

We explore mechanisms for the regulation of star formation in dwarf galaxies. We concentrate primarily on a sample in the Virgo cluster, which has HI and blue total photometry, for which we collected H$\alpha$ data at the Wise Observatory.…

天体物理学 · 物理学 2009-10-30 Noah Brosch , Ana Heller , Elchanan Almoznino

We investigate the environmental dependence of galaxies with star formation from a volume-limited sample of 4782 nearby field galaxy spectra extracted from the 2dF Galaxy Redshift Survey final data release. The environment is characterized…

天体物理学 · 物理学 2009-11-10 Abilio Mateus , Laerte Sodre

The location of HII regions, which indicates the locus of present star formation in galaxies, is analyzed for a large collection of 110 irregular galaxies (Irr) imaged in H$\alpha$ and nearby continuum. The analysis is primarily by visual…

天体物理学 · 物理学 2015-06-24 Noah Brosch , Ana Heller , Elchanan Almoznino

Neutral intergalactic clouds are so greatly out numbered by galaxies that their integral HI content is negligible in comparison to that contained in optically luminous galaxies. In fact, no HI cloud that is not associated with a galaxy or…

天体物理学 · 物理学 2007-05-23 F. H. Briggs
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