LEDA 35178 , the SIMBAD biblio

LEDA 35178 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:23:33


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Title First 3 Authors
1987ApJS...63..265W 513 103 Neutral hydrogen in compact groups of galaxies. WILLIAMS B.A. and ROOD H.J.
1989ApJS...70..687H viz 14       D               1 487 192 A photometric catalog of compact groups of galaxies. HICKSON P., KINDL E. and AUMAN J.R.
1992ApJ...399..353H viz 14       D               1 569 344 Dynamical properties of compact groups of galaxies. HICKSON P., MENDES DE OLIVEIRA C., HUCHRA J.P., et al.
1993Ap&SS.209..181A 232 4 On actual presence of discordant-redshift galaxies in compact groups. ANOSOVA J. and KISELEVA L.
1995MNRAS.273..139M 54 20 The nature of discordant redshift galaxies in compact groups. MENDES DE OLIVEIRA C.
1996A&AS..117..467G viz 22335 19 An image database. II. Catalogue between δ=-0deg and δ=70deg. GARNIER R., PATUREL G., PETIT C., et al.
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2003AJ....126.2152R viz 15       D               15140 214 CAIRNS: the cluster and infall region nearby survey. I. Redshifts and mass profiles. RINES K., GELLER M.J., KURTZ M.J., et al.
2015ApJ...812...89M viz 16       D               1 12670 7 ECO and RESOLVE: galaxy disk growth in environmental context. MOFFETT A.J., KANNAPPAN S.J., BERLIND A.A., et al.
2017ApJ...837..120G viz 16       D               1 14403 66 LOSS revisited. I. Unraveling correlations between supernova rates and galaxy properties, as measured in a reanalysis of the Lick Observatory Supernova Search. GRAUR O., BIANCO F.B., HUANG S., et al.
2017ApJ...849...20E viz 16       D               2 9926 2 The baryonic collapse efficiency of galaxy groups in the RESOLVE and ECO surveys. ECKERT K.D., KANNAPPAN S.J., LAGOS C.D.P., et al.
2020MNRAS.494.1784A viz 17       D               1 47437 9 Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. ASMUS D., GREENWELL C.L., GANDHI P., et al.

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