LEDA 8191 , the SIMBAD biblio

LEDA 8191 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST09:16:23


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
1992PNAOJ...2..399T viz 464 5 Kiso survey for ultraviolet-excess galaxies. XV. TAKASE B. and MIYAUCHI-ISOBE N.
2009MNRAS.393.1531G viz 15       D               1 906 423 Structural properties of pseudo-bulges, classical bulges and elliptical galaxies: a Sloan Digital Sky Survey perspective. GADOTTI D.A.
2010MNRAS.405..783M viz 15       D               1 5435 245 Galaxy Zoo: passive red spirals. MASTERS K.L., MOSLEH M., ROMER A.K., et al.
2014ApJ...788...45T viz 16       D               1 224162 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2015A&A...584A..88F viz 16       D               1 568 6 Central enhancement of the nitrogen-to-oxygen abundance ratio in barred galaxies. FLORIDO E., ZURITA A., PEREZ I., et al.
2016MNRAS.457.2703R viz 16       D               1 3319 14 Local SDSS galaxies in the Herschel Stripe 82 survey: a critical assessment of optically derived star formation rates. ROSARIO D.J., MENDEL J.T., ELLISON S.L., et al.
2017A&A...599A..71D viz 16       D               1 209270 41 Aperture-free star formation rate of SDSS star-forming galaxies. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2019MNRAS.487.5572M viz 17       D               1 4573 ~ Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies. MISHRA P.K., WADADEKAR Y. and BARWAY S.
2020MNRAS.493...87T viz 17       D               1 988 46 A physically motivated definition for the size of galaxies in an era of ultradeep imaging. TRUJILLO I., CHAMBA N. and KNAPEN J.H.
2022A&A...666A.186D viz 18       D               1 194358 6 Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.

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