Results 81 to 90 of about 3,788 (174)
The dynamics of the bulge dominated galaxy NGC 7814 in MOND
, 2012 Context. The bulge dominated galaxy NGC 7814 provides one of the strongest dynamical tests possible for MOdified Newtonian Dynamics (MOND). Spitzer 3.6 μm photometry fixes the bulge parameterisation and strongly constrains the properties of the ...
K. J. van der Heyden +2 more
core +1 more source
, 2008 While galactic bulges may contain no significant dust of their own, the dust within galaxy discs can strongly attenuate the light from their embedded bulges.
Alister Graham (18926479) +1 more
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The nuclear bulge of the Galaxy - III. Large-scale physical characteristics of stars and interstellar matter [PDF]
, 2002 We analyse IRAS and COBE DIRBE data at wavelengths between 2.2 and 240 mum of the central 500 pc of the Galaxy and derive the large-scale distribution of stars and interstellar matter in the Nuclear Bulge.
Launhardt, R. +5 more
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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)
openaire +2 more sources
, 2010 International audienceExploring the in-plane region of our Galaxy is an interesting but challenging quest, because of the complex structure and the highly variable extinction. We here analyse photometric near-infrared data using the Besançon Galaxy Model
Marshall, D. J. +3 more
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Examining Galaxy Bulge Regions with the Sloan Digital Sky Survey
Nearly all of the ordinary matter in the universe is located in galaxies, which are made up stars, gas, dust, and black holes, and range in size from a few thousand to a few hundred thousand light years across. Galaxies come in different shapes, but many
Maller, Ariyeh, Draves, Sarah E
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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.
wiley +1 more source
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
openaire +3 more sources
The Puzzling Bulge to Disk Nova Ratio in the Andromeda Galaxy (M31)
, 2016 Novae in M31 are often associated with the bulge component of the light from this galaxy, i.e., more novae are assumed to be produced in the bulge of M31.
Kaur, Amanpreet
core +1 more source
Lenticular galaxy formation: possible luminosity dependence [PDF]
, 2007 We investigate the correlation between the bulge effective radius (re ) and disk scale length (rd ) in the near-infrared K band for lenticular galaxies in the field and in clusters.
YALIA DIVAKARA MAYYA
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