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We present preliminary results of a long-term study aimed at answering a number of open questions on the evolution of starbursts in local galaxies. The project employes mainly HST data from the ultraviolet to the red of the stellar…

Astrophysics · Physics 2007-05-23 Daniela Calzetti , Jason Harris

We investigate the role of stellar mass in shaping the intrinsic thickness of galaxy discs by determining the probability distribution of apparent axis ratios (b/a) for two different samples that probe the faint end of the galaxy luminosity…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 R. Sanchez-Janssen , J. Mendez-Abreu , J. A. L. Aguerri

Dwarf galaxies play an important role in our understanding of galaxy formation and evolution, and starbursts are believed to strongly affect their structure and evolution. Here we present a study of 12 of the nearest dwarf galaxies thought…

Astrophysics · Physics 2009-10-31 Amanda T. Marlowe , Gerhardt R. Meurer , Timothy M. Heckman

The results of UBV and H alpha imaging of a large sample of isolated dwarf irregular galaxies are interpreted in the context of composite stellar population models. The observed optical colors are best fit by composite stellar populations…

Astrophysics · Physics 2009-08-17 L. van Zee

Starbursts are episodes of intense star-formation in the central regions of galaxies, and are the sites of roughly 25% of the high-mass star-formation in the local universe. In this contribution I review the role starbursts play in the…

Astrophysics · Physics 2009-10-31 Timothy M. Heckman

The formation of globular clusters remains an open debate. Dwarf starburst galaxies are efficient at forming young massive clusters with similar masses as globular clusters and may hold the key to understanding their formation. We study…

We present millimeter molecular-line complemented by optical observations, along with a reanalysis of archival centimeter HI and continuum data, to infer the global dynamics and determine where dense molecular gas and massive stars…

Astrophysics of Galaxies · Physics 2015-06-15 Hsi-An Pan , Jeremy Lim , Satoki Matsushita , Tony Wong , Stuart Ryder

Recent photometric observations by the {\it Hubble Space Telescope (HST)} have revealed the physical properties of stellar galactic nuclei in nucleated dwarf galaxies in the Virgo cluster of galaxies. In order to elucidate the formation…

Astrophysics · Physics 2009-11-11 Kenji Bekki , Warrick J. Couch , Yasuhiro Shioya

The origin of the observed steep rotation curves of blue compact dwarf galaxies (BCDs) remains largely unexplained by theoretical models of BCD formation. We therefore investigate the rotation curves in BCDs formed from mergers between…

Astrophysics of Galaxies · Physics 2016-09-14 A. Watts , K. Bekki

Observations have revealed prodigious amounts of star formation in starburst galaxies as traced by dust and molecular emission, even at large redshifts. Recent work shows that for both nearby spiral galaxies and distant starbursts, the…

Blue Compact Dwarf and Dwarf Irregular galaxies are generally believed to be unevolved objects, due to their blue colors, compact appearance and large gas fractions. Many of these objects show an ongoing intense burst of star formation or…

Astrophysics · Physics 2007-05-23 S. Recchi , G. Hensler

Irregular (Irr) galaxies are gas-rich objects with recent or ongoing star formation. In absence of spiral density waves, star formation occurs largely stochastically. The scattered star-forming regions tend to be long-lived and migrate…

Astrophysics · Physics 2007-05-23 Eva K. Grebel

We investigate the role of stellar mass in shaping the intrinsic thickness of faint systems by determining the probability distribution of apparent axis ratios for two different samples that probe the faint end of the galaxy luminosity…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-16 R. Sánchez-Janssen , J. Méndez-Abreu , J. A. L. Aguerri

I review the evolutionary status of the field populations of starbursting dwarf galaxies and low surface brightness spirals. Particular attention is paid to the long standing problem of the progenitors for star burst galaxies, which may be…

Astrophysics · Physics 2007-05-23 Stacy S. McGaugh

Crucial to a quantitative understanding of galaxy evolution are the properties of the inter-stellar medium that regulate galactic-scale star formation activity. We present here the results of a suite of star formation models applied to the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 E C Elson , W J G de Blok , R C Kraan-Korteweg

We present N-body/SPH simulations of the evolution of an isolated dwarf galaxy including a detailed model for the ISM, star formation and stellar feedback. Depending on the strength of the feedback, the modelled dwarf galaxy shows periodic…

Astrophysics · Physics 2009-11-10 F. I. Pelupessy , P. P. van der Werf , V. Icke

We present the results of high spatial resolution HI observations of five intrinsically compact dwarf galaxies which are currently experiencing a strong burst of star formation. The HI maps indicate that these systems have a complex and…

Astrophysics · Physics 2009-10-30 L. van Zee , E. D. Skillman , J. J. Salzer

Due to their low gravitational energies, dwarf galaxies are greatly exposed to energetical influences from internal and external sources. By means of chemodynamical models we show that their star formation is inherently self-regulated, that…

Astrophysics · Physics 2009-11-11 S. Recchi , G. Hensler

Starburst galaxies have a highly increased star-formation rate compared to regular galaxies and inject huge amounts of kinetic power into the interstellar medium via supersonic stellar winds, and supernova explosions. Supernova remnants,…

High Energy Astrophysical Phenomena · Physics 2016-07-20 Stefan Ohm

We report the measured H$\alpha$ fluxes and images of 66 nearby objects observed with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. Three of these objects: IC2233, UGC4704, and NGC3432 are…

Astrophysics of Galaxies · Physics 2019-05-01 S. S. Kaisin , I. D Karachentsev