Results 91 to 100 of about 1,381 (128)
WLM: Dynamics of an isolated dwarf irregular galaxy under ram pressure in the Local Group
Neel Kolhe +7 more
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Morphology and kinematics of interacting galaxies : the spheroidal + irregular pairs
C. F. McCain
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Mass-to-Light versus Color Relations for Dwarf Irregular Galaxies
Kimberly A. Herrmann +3 more
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Magnetic Field Structure and Young Stellar Populations in the Irregular Galaxy NGC 4449
Yenice, Efe, Çevirgen, Ahmet Selim
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Star Formation in Irregular Galaxies
Science, 1989Irregular galaxies can be viewed as laboratories for studying the processes of star formation. This class of galaxy, unlike the more familiar spiral galaxies, forms stars without spiral arms and does so from a chemically less-evolved interstellar medium.
D A, Hunter, J S, Gallagher
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The Kinematics of Spiral and Irregular Galaxies
Annual Review of Astronomy and Astrophysics, 1978The present status of kinematical studies of intermediate- and late-type galaxies is reviewed. The emphasis is on observations that result in extensive maps of velocity fields rather than determinations of rotation curves from major axis observations only.
P. C. van der Kruit, R. J. Allen
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Structure and Evolution of Irregular Galaxies
Annual Review of Astronomy and Astrophysics, 1984Proprietes fondamentales: lumiere, masses et cinematique, abondances, populations stellaires. Proprietes de la formation stellaire: taux de formation stellaire, distribution des regions de formation stellaire, les complexes de formation stellaire et le milieu interstellaire, la fonction de masse initiale, le gaz utilisable.
John S. Gallagher, Deidre A. Hunter
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Starbursts in Ring and Irregular Galaxies
Publications of the Astronomical Society of Australia, 1991AbstractThis paper presents the current status of a Ph.D. project undertaken to search for extended-scale bursts of star formation (> 1 kpc) in irregular and collisionally produced ring galaxies, principally in the southern half of the sky. Results of recent 8.4 GHz radio continuum observations and UBVRI CCD imaging of some of the program galaxies ...
V. J. McIntyre, W. J. Zealey
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2004
Dwarf irregular galaxies at optical wavelengths are small, faint and appear to be unstructured and irregular in shape. They are typically gas-rich, metal-poor systems, with varying levels of STAR FORMATION occurring in a haphazard manner across the ...
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Dwarf irregular galaxies at optical wavelengths are small, faint and appear to be unstructured and irregular in shape. They are typically gas-rich, metal-poor systems, with varying levels of STAR FORMATION occurring in a haphazard manner across the ...
openaire +2 more sources

