Works matching IS 05717256 AND DT 2012 AND VI 55 AND IP 3
Results: 14
Morphology and color indices of galaxies in Pairs: Criteria for the classification of galaxies.
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- Astrophysics, 2012, v. 55, n. 3, p. 293, doi. 10.1007/s10511-012-9236-7
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Analytic solution for kinetic equilibrium with respect to β-processes in nucleon plasmas with relativistic pairs.
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- Astrophysics, 2012, v. 55, n. 3, p. 387, doi. 10.1007/s10511-012-9245-6
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X-ray and very high energy gamma-ray observations of the galaxy Mrk 501 during May-June, 2006.
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- Astrophysics, 2012, v. 55, n. 3, p. 325, doi. 10.1007/s10511-012-9239-4
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Infrared spectral properties of wolf-rayet galaxies.
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- Astrophysics, 2012, v. 55, n. 3, p. 306, doi. 10.1007/s10511-012-9237-6
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- Article
Radial system of dark globules in Ser OB2.
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- Astrophysics, 2012, v. 55, n. 3, p. 363, doi. 10.1007/s10511-012-9242-9
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New bright carbon stars found in the DFBS.
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- Astrophysics, 2012, v. 55, n. 3, p. 424, doi. 10.1007/s10511-012-9248-3
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Magnetic fields of chemically peculiar stars.
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- Astrophysics, 2012, v. 55, n. 3, p. 334, doi. 10.1007/s10511-012-9240-y
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Energy source for the radio emission from pulsars.
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- Astrophysics, 2012, v. 55, n. 3, p. 377, doi. 10.1007/s10511-012-9244-7
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- Article
Light curves, variations in the MgII h and k and MgI (2852 Å) emission lines, and polarization of light from the mirids.
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- Astrophysics, 2012, v. 55, n. 3, p. 351, doi. 10.1007/s10511-012-9241-x
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Medium resolution spectroscopy of the supergiant O31f Cyg OB2 No. 7.
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- Astrophysics, 2012, v. 55, n. 3, p. 371, doi. 10.1007/s10511-012-9243-8
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Initial phase of protostar formation.
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- Astrophysics, 2012, v. 55, n. 3, p. 397, doi. 10.1007/s10511-012-9246-5
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Spatial distribution of a time-harmonic wave field scattered by a one-dimensional medium.
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- Astrophysics, 2012, v. 55, n. 3, p. 411, doi. 10.1007/s10511-012-9247-4
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- Article
Electrons in quark plasmas.
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- Astrophysics, 2012, v. 55, n. 3, p. 429, doi. 10.1007/s10511-012-9249-2
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- Article
Relationship between the infrared and radio emission of wolf-rayet galaxies.
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- Astrophysics, 2012, v. 55, n. 3, p. 317, doi. 10.1007/s10511-012-9238-5
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- Article