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On the Luminosity Class of Late-Type Spiral Galaxies
Publications of the Astronomical Society of Japan, 1976Abstract Correlations between the luminosity class in the DDO system and several observational quantities are investigated for late-type spiral galaxies. The luminosity class is found to be well correlated with maximum rotational velocity log Vm (correlation coefficient –0.83), Holmberg’s (1958) photometric radius log RH(–0.80), and ...
Masanori Iye, Keiichi Kodaira
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The History of Star Formation in Normal Late-Type Galaxies
Astrophysics and Space Science, 2001We study the history of star formation of late-type galaxies using a multi-frequency analysis of a large sample of nearby objects spanning a wide range of morphological types and luminosities. The history of star formation and the total amount of gas of a galaxy are found to depend primarily on the total mass and only secondarily on the morphological ...
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Dark Matter in Late-Type Galaxies
1992The status of our knowledge of the extent and distribution of dark matter in late-type galaxies is reviewed. Recent attempts to alleviate the need for dark matter in late-type galaxies are examined, but none are found to give a satisfactory explanation. The mass distribution and shapes of dark matter halos are still known only poorly.
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Gaseous Halos of Late-Type Spiral Galaxies
Publications of the Astronomical Society of the Pacific, 1997This article reviews the most recent observational results on disk-halo interactions in nearby galaxies. The implications of these results on our understanding of the structure of the interstellar medium (ISM) in our Galaxy and external spiral galaxies, with particular emphasis on the halo ISM, are discussed. Disk-halo interactions occur only above the
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Dark Halos around Late-type galaxies
1985In order to investigate the mass-to-light ratio in irregular Magellanic galaxies, a sample of 21 Sdm, Sm, Im objects, for which high-resolution velocity fields observed in 21 cm line are available in the literature, has been selected. Rotation curves, either taken from the authors or reconstructed from the original data and sometimes supplemented with ...
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The formation of stellar halos in late-type galaxies
2007Near–field observations may provide tight constraints - i.e. 'boundary conditions' - on any model of structure formation in the Universe. Detailed observational data have long been available for the Milky Way (e.g., Freeman and Bland-Hawthorn 2002) and have provided tight constraints on several Galaxy formation models (e.g.: Abadi et al.
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Non-circular flows in HIghMass galaxies in a test of the late accretion hypothesis
Monthly Notices of the Royal Astronomical Society, 2021Martha Haynes +2 more
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The information on halo properties contained in spectroscopic observations of late-type galaxies
Monthly Notices of the Royal Astronomical Society, 2023Adrianne Slyz +2 more
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The physical properties of local (U)LIRGs: A comparison with nearby early- and late-type galaxies
Astronomy and Astrophysics, 2021Angelos Nersesian +2 more
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The multi-phase gaseous halos of star-forming late-type galaxies
Astronomy and Astrophysics, 2006Ralf-Juergen Dettmar, D Breitschwerdt
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