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Galaxy disks and disk galaxies
2001This volume presents the proceedings of the conference "Galaxy Disks and Disk Galaxies", sponsored by the Vatican Observatory. The meeting was held in Rome from 12 to 16 June, 2000, the Jubilee Year, a special year for the Catholic Church. The venue of the meeting was the Pontifical Gregorian University, a descendant of the former Roman College where ...
FUNES J. G., CORSINI, ENRICO MARIA
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The Formation of Disks in Galaxies
1992Different chemo-dynamical models dealing with the formation of stellar disks in the course of galaxy evolution are presented. One-dimensional models concerning the vertical stratification of disks are in strikingly good agreement with the solar vicinity.
G. Hensler +4 more
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1992
The outermost gaseous disk of our Galaxy is warped (Burton and te Lintel Hekkert 1986; Wouterloot et al. 1990), and a stellar component may be present as well (Miyamoto et al. 1988; Djorgovski and Sosin 1989). If so, the outermost edges of the Galaxy’s disk may be more readily studied using the warp than relying upon the terribly crowded and nearly to ...
Bruce W. Carney, Patrick Seitzer
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The outermost gaseous disk of our Galaxy is warped (Burton and te Lintel Hekkert 1986; Wouterloot et al. 1990), and a stellar component may be present as well (Miyamoto et al. 1988; Djorgovski and Sosin 1989). If so, the outermost edges of the Galaxy’s disk may be more readily studied using the warp than relying upon the terribly crowded and nearly to ...
Bruce W. Carney, Patrick Seitzer
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Photometry of Disks in Galaxies
1989In this review, four aspects of the light distribution in galactic disks are addressed: (1) Following the pioneering work by de Vaucouleurs in the 1950’s, we know that the majority of disks have a radial surface brightness distribution that follows an exponential law.
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1997
As astronomers involved in studies of interstellar dust in various environments are about to head into ISO’s decade, it seems to me both a good and a risky idea to try and summarize our current knowledge of the properties of dust in galactic disks. Indeed it is always interesting to sort out our various findings to see which questions were answered ...
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As astronomers involved in studies of interstellar dust in various environments are about to head into ISO’s decade, it seems to me both a good and a risky idea to try and summarize our current knowledge of the properties of dust in galactic disks. Indeed it is always interesting to sort out our various findings to see which questions were answered ...
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High star formation rates as the origin of turbulence in early and modern disk galaxies
Nature, 2010Andrew W Green +2 more
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Stellar Disk Evolution and Gaseous Disk Turbulence of Dwarf Irregular Galaxies
Springer Theses, 2016Hong-Xin Zhang
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