Star Formation in Normal Irregular Galaxies [PDF]
Normal, non-interacting irregular galaxies can be quite successful at forming stars. Therefore, spiral density waves are not necessary to a vigorous production of stars. Nevertheless, there is a large range in star-formation rates among irregular galaxies.
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Distinguishing galaxies as either fast or slow rotators plays a vital role in understanding the processes behind galaxy formation and evolution. Standard techniques, which are based on the λR spin parameter obtained from stellar kinematics, frequently ...
Amirmohammad Chegeni +4 more
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FIGGS: Faint Irregular Galaxies GMRT Survey – overview, observations and first results [PDF]
Ayesha Begum +4 more
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Chemical evolution of irregular galaxies
10 pages, 3 figs, uses moriond.sty. Review presented at XVIIIth Rencontre de Moriond `Dwarf Galaxies and Cosmology', eds.
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Star Formation Histories of the LEGUS Dwarf Galaxies. II. Spatially Resolved Star Formation History of the Magellanic Irregular NGC 4449∗ [PDF]
E. Sacchi +18 more
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An Arecibo 327 MHz Search for Radio Pulsars and Bursts in the Dwarf Irregular Galaxies Leo A and T [PDF]
F. Crawford, Kohei Hayashi
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FEAST: Probing the Stellar Population of the Starburst Dwarf Galaxy NGC 4449 with JWST/NIRCam
We present new JWST/NIRCam observations of the starburst irregular galaxy NGC 4449, obtained in Cycle 1 as part of the Feedback in Emerging extrAgalactic Star clusTers program, which we use to investigate its resolved stellar populations and their ...
Matteo Correnti +24 more
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Constraining the Milky Way potential using the dynamical kinematic substructures
We present a method to constrain the potential of the non-axisymmetric components of the Galaxy using the kinematics of stars in the solar neighborhood. The basic premise is that dynamical substructures in phase-space (i.e.
Antoja T., Monari G., Helmi A.
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SPECTRAL: A new evolutionary synthesis code. Application to the irregular Galaxy NGC 1560 [PDF]
Gerardo A. Vázquez +2 more
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Morphology of star formation regions in irregular galaxies [PDF]
N. Brosch, Ana Heller, E. Almoznino
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