Results 1 to 10 of about 37,993 (251)
Supernova Remnants in the Irregular Galaxy NGC 4449
The nearby irregular galaxy NGC 4449 has a star formation rate of ∼0.4 M _☉ yr ^−1 and should host of order 70 supernova remnants (SNRs) younger than 20,000 yr, a typical age for SNRs expanding into an interstellar medium (ISM) with a density of 1 cm ^−3
P. Frank Winkler +2 more
doaj +3 more sources
The oxygen abundance deficiency in irregular galaxies [PDF]
The observed oxygen abundances in a number of irregular galaxies have been compared with predictions of the closed-box model of chemical and photometric evolution of galaxies. Oxygen is found to be deficient with respect to the predicted abundances. This
Ferrini, F., Pilyugin, L. S.
core +4 more sources
Stellar structure of irregular galaxies: Edge-on galaxies [PDF]
13 pages, 7 ...
N. A. Tikhonov
openalex +4 more sources
Lopsidedness in dwarf irregular galaxies [PDF]
We quantify the amplitude of the lopsidedness, the azimuthal angular asymmetry index, and the concentration of star forming regions, as represented by the distribution of the H$\alpha$ emission, in a sample of 78 late-type irregular galaxies.
Abraham +41 more
core +5 more sources
Diffuse Ionized Gas in the Dwarf Irregular Galaxy DDO 53
The spectral characteristics throughout the dwarf irregular galaxy DDO 53 are studied. The results are very similar to those for other irregular galaxies: high excitation and low values of the [SII]/Halpha ratio.
A. M. Hidalgo-Gámez +12 more
exaly +3 more sources
FIGGS Faint Irregular Galaxies GMRT Survey [PDF]
The Faint Irregular Galaxies GMRT Survey (FIGGS) is a large program aimed at providing a comprehensive and statistically robust characterisation of the neutral ISM properties of faint (M_B > -14.5), nearby, gas rich, dwarf irregular galaxies using the Giant Metrewave Radio Telescope (GMRT). Here we briefly describe the survey and discuss some of the
Ayesha Begum +4 more
openalex +4 more sources
WLM: Dynamics of an isolated dwarf irregular galaxy under ram pressure in the Local Group
The Wolf–Lundmark–Melotte (WLM) galaxy is an archetypal dwarf irregular galaxy that has not experienced interactions with major Local Group galaxies within the past 8 Gyr.
Kolhe Neel +7 more
doaj +3 more sources
LBT/MODS spectroscopy of globular clusters in the irregular galaxy NGC 4449 [PDF]
F Annibali, E Morandi, Laura L Watkins
exaly +2 more sources
Stellar population of the irregular galaxy IC 10 [PDF]
Based on our observations with the 6-m BTA telescope at the Special Astrophysical Observatory, the Russian Academy of Sciences, and archival Hubble Space Telescope images, we have performed stellar photometry for several regions of the irregular galaxy IC 10, a member of the Local Group.
N A Tikhonov, O A Galazutdinova
exaly +3 more sources
The Sculptor dwarf irregular galaxy SDIG: present and past [PDF]
C A Heisler +2 more
exaly +2 more sources

