Results 21 to 30 of about 12,615 (238)

THE INTRINSIC PROPERTIES OF SDSS GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2009
The observed properties of galaxies vary with inclination; for most applications we would rather have properties that are independent of inclination, intrinsic properties. One way to determine inclination corrections is to consider a large sample of galaxies, study how the observed properties of these galaxies depend on inclination and then remove this
Maller, Ariyeh H.   +3 more
openaire   +2 more sources

DEPENDENCE OF BARRED GALAXY FRACTION ON GALAXY PROPERTIES AND ENVIRONMENT [PDF]

open access: yesThe Astrophysical Journal, 2012
20 pages, 18 figures, accepted for publication in ...
Lee, Gwang-Ho   +3 more
openaire   +2 more sources

Properties of GRB host galaxies

open access: yesFourth Huntsville gamma-ray burst symposium, 1998
5 pages, AIPPROC LaTeX, to appear in "Gamma-Ray Bursts, 4th Huntsville Symposium," eds. C. Meegan, R.
Hartmann, Dieter H., Band, David L.
openaire   +3 more sources

Galaxy and Mass Assembly (GAMA): merging galaxies and their properties [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
14 pages, 8 figures, MNRAS ...
De Propris, Roberto   +9 more
openaire   +8 more sources

The clustering properties of faint galaxies

open access: yesThe Astrophysical Journal, 1995
The two-point angular correlation function of galaxies, \wte, has been computed from a new survey of faint galaxies covering a 2 deg$^2$ area near the North Galactic Pole. This survey, which is complete to limiting magnitudes \jmag=24 and \fmag=23, samples angular scales as large as $1\degpoint5$.
Infante, L., Pritchet, C. J.
openaire   +2 more sources

Two-phase galaxy formation: the evolutionary properties of galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2010
We use our model for the formation and evolution of galaxies within a two-phase galaxy formation scenario, showing that the high-redshift domain typically supports the growth of spheroidal systems, whereas at low redshifts the predominant baryonic growth mechanism is quiescent and may therefore support the growth of a disc structure.
Cook, Michael   +4 more
openaire   +3 more sources

Galaxy and Mass Assembly (GAMA): Low-redshift Quasars and Inactive Galaxies Have Similar Neighbors

open access: yesThe Astrophysical Journal, 2023
We explore the properties of galaxies in the proximity (within a ∼2 Mpc radius sphere) of Type I quasars at 0.1 < z
Maria B. Stone   +7 more
doaj   +1 more source

ORBITAL DEPENDENCE OF GALAXY PROPERTIES IN SATELLITE SYSTEMS OF GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2010
12 pages, 18 figures.
Hwang, Ho Seong, Park, Changbom
openaire   +2 more sources

Modelling the extinction properties of galaxies

open access: yesAstrophysics and Space Science, 2001
Recently (Granato, Lacey, Silva et al. 2000, astro-ph/0001308) we have combined our spectrophotometric galaxy evolution code which includes dust reprocessing (GRASIL, Silva et al. 1998) with semi-analytical galaxy formation models (GALFORM, Cole et al. 1999).
Granato, G. L.   +6 more
openaire   +2 more sources

The 2dF galaxy redshift survey: clustering properties of radio galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2004
10 pages, 8 figures, minor changes, to appear on ...
Magliocchetti, Manuela   +27 more
openaire   +5 more sources

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