Results 21 to 30 of about 34 (34)
A Catalog of the Most Optically Luminous Galaxies at z < 0.3: Super Spirals, Super Lenticulars, Super Post-mergers, and Giant Ellipticals [PDF]
The Astrophysical Journal Supplement Series, 2019 We present a catalog of the 1525 most optically luminous galaxies from the Sloan Digital Sky Survey (SDSS) with r-band luminosity L_r > 8L* and redshift z<0.3, including 84 super spirals, 15 super lenticulars, 14 super post-merger galaxies, and 1400 giant ellipticals.
Patrick M. Ogle +4 more
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Isophotal shapes of elliptical/lenticular galaxies from the Sloan Digital Sky Survey
Monthly Notices of the Royal Astronomical Society, 2006 25 pages, 22 figures, accepted for publication in MNRAS. Revised to match the final version accepted for publication in MNRAS.
C. N. Hao +5 more
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Journal of Education and ScienceThe Fundamental Plane relates the effective radius and surface brightness of an early-type galaxy to its velocity dispersion. It is important in understanding galaxy formation and evolution processes. The present work aims to investigate this relation as well as Faber-Jackson and Kormendy relations for both elliptical and lenticular galaxies separately
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Investigating the Correlations between Physical Parameters of Elliptical and Lenticular Galaxies
Iraqi Journal of ScienceThis study aims to investigate the features of stellar-gaseous kinematics and dynamics mass using scaling coefficient relationships (such as the Faber–Jackson relation (FJR)) of two samples of elliptical and lenticular galaxies. These two samples of 80 ellipticals and 97 lenticulars were selected from previous literature works.
Rabab Mozher J., Mohammed Naji Al Najm
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The dwarf star content of elliptical and lenticular galaxies
The Astrophysical Journal, 1986 N. Visvanathan, A. J. Pickles, D. Carter
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Dust-lanes in elliptical and lenticular galaxies
, 1982 A small proportion of elliptical and lenticular galaxies show evidence of well-defined dust-lanes when examined on deep survey plates. New near-infrared (JHK) observations of 46 dust-lane galaxies are presented and compared with those for a sample of 24 morphologigally normal systems. Infrared excesses are found preferentially in galaxies which exhibit
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Monthly Notices of the Royal Astronomical SocietyABSTRACT In a recent series of papers, supermassive black holes were used to discern pathways in galaxy evolution. By considering the black holes’ coupling with their host galaxy’s bulge/spheroid, the progression of mass within each component has shed light on the chronological sequence of galaxy speciation.
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Erratum: Isophotal shapes of elliptical/lenticular galaxies from the Sloan Digital Sky Survey [PDF]
Monthly Notices of the Royal Astronomical Society, 2006 C. N. Hao +4 more
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In a recent series of papers, supermassive black holes were used to discern pathways in galaxy evolution. By considering the black holes' coupling with their host galaxy's bulge/spheroid, the progression of mass within each component has shed light on the chronological sequence of galaxy speciation.
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Publications of the Astronomical Society of the Pacific, 2000
The Virgo Cluster of galaxies is a complex system composed of several subclusters or ““ clouds.II Our understanding of this structure is severely limited by the small number of member galaxies for which high-precision distance measurements are available.
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The Virgo Cluster of galaxies is a complex system composed of several subclusters or ““ clouds.II Our understanding of this structure is severely limited by the small number of member galaxies for which high-precision distance measurements are available.
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