Results 61 to 70 of about 121 (116)
The nuclei of bulge-less galaxies [PDF]
, 2004 Als Beitrag zur Vervollst?andigung unseres Wissens ?uber Galaxienzentren wurde die Zentral-Region sehr sp?ater (bulge-loser) Spiralgalaxien untersucht.
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Galaxy Zoo: The Environmental Dependence of Bars and Bulges in Disc Galaxies
, 2011 We present an analysis of the environmental dependence of bars and bulges in disc galaxies, using a volume-limited catalogue of 15810 galaxies at z<0.06 from the Sloan Digital Sky Survey with visual morphologies from the Galaxy Zoo 2 project. We find that the likelihood of having a bar, or bulge, in disc galaxies increases when the galaxies have ...
Skibba, Ramin A. +10 more
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Extinction Effects on Galaxy Counts for Bulge‐Disk Galaxies
The Astrophysical Journal, 1997 We examine extinction effects of interstellar dust on galaxy counts for bulge-disk galaxies. Evolution of dust mass is calculated simultaneously with galaxy chemical evolution equations under the context of the so-called infall model, and three-dimensional radiative transfer calculation is performed with scattering effects. Prevailing importance of the
V. Vansevičius, N. Arimoto, K. Kodaria
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Spheroid and disk signatures in galaxy bulges* [PDF]
EAS Publications Series, 2003 Review at JENAM2002 Galaxy Dynamics Workshop (Porto, Portugal, 2002 September 3-7).
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Galaxy Bulges and Elliptical Galaxies - Lecture Notes
, 2012 In press; 16 pages, 15 figures; notes to the PhD School of Astrophysics "F. Lucchin", held in Erice, Italy, September 2011; G. Bono, M. Zoccali (eds.)
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The Central kpc of Galaxy Bulges
, 2001 6 pages, 3 figures. Contributed paper to "The Central kpc of Starbursts and AGN: the La Palma connection'', Eds. J.H. Knapen, J.E. Beckman, I. Shlosman and T.J. Mahoney, ASP conf. series, in press (2001)
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Galaxy Bulges and Their Massive Black Holes: A Review [PDF]
, 2016 With references to both key and oft-forgotten pioneering works, this article starts by presenting a review into how we came to believe in the existence of massive black holes at the centres of galaxies. It then presents the historical development of the near-linear (black hole)-(host spheroid) mass relation, before explaining why this has recently been
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87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
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Merger History of Galaxies and Disk+Bulge Formation
, 2009 We discuss the transitions of galaxy morphologies within the CDM paradigm under the assumption of bulge formation in mergers and disk growth via cooling of gas and subsequent star formation. Based on the relative importance of these two competing processes it is possible to make predictions on the expected morphological mix of galaxies.
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