MCG+07-07-003 , the SIMBAD biblio

MCG+07-07-003 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST16:54:05

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1996A&A...309..749P viz 1603 202 The fundamental plane of early-type galaxies: stellar populations and mass-to-light ratio. PRUGNIEL P. and SIMIEN F.
1998AJ....116.2108K viz 178 15 A photometric and kinematic study of AWM 7. KORANYI D.M., GELLER M.J., MOHR J.J., et al.
2000AJ....119...44K viz 493 25 Kinematics and mass profile of AWM 7. KORANYI D.M. and GELLER M.J.
2002AJ....123..100K viz 1581 23 Kinematics of AWM and MKW poor clusters. KORANYI D.M. and GELLER M.J.
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.
2003ApJ...596..181F 10 24 Chandra observation of the core of the galaxy cluster AWM 7. FURUSHO T., YAMASAKI N.Y. and OHASHI T.
2013MNRAS.432.1680Y 55       D     X         2 26 23 Locations of peculiar supernovae as a diagnostic of their origins. YUAN F., KOBAYASHI C., SCHMIDT B.P., et al.
2013MNRAS.434..527L 156           X         4 72 40 Environment-derived constraints on the progenitors of low-luminosity type I supernovae. LYMAN J.D., JAMES P.A., PERETS H.B., et al.
2014MNRAS.444.2157L 16       D               1 34 23 The progenitors of calcium-rich transients are not formed in situ. LYMAN J.D., LEVAN A.J., CHURCH R.P., et al.
2015MNRAS.452.2463F 119           X         3 39 28 Kinematics and host-galaxy properties suggest a nuclear origin for calcium-rich supernova progenitors. FOLEY R.J.
2016MNRAS.458.1768L 121           X C       2 18 18 Hubble Space Telescope observations of the host galaxies and environments of calcium-rich supernovae. LYMAN J.D., LEVAN A.J., JAMES P.A., 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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