Autor:
Pan, H.-A.
Lin, L.
Hsieh, B.-C.
Sánchez, S.F.
Ibarra-Medel, H.
Boquien, M.
Lacerna, I.
Argudo-Fernández, M.
Bizyaev, D.
Cano-Díaz, M.
Drory, N.
Gao, Y.
Masters, K.
Pan, K.
Tabor, M.
Tissera, P.
Xiao, T.
The galaxy integrated Hα star formation rate-stellar mass relation, or SFR(global)-M ∗(global) relation, is crucial for understanding star formation history and evolution of galaxies. However, many studies have dealt with SFR using unresolved measurements, which makes it difficult to separate out...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/6760
Pan, H.-A.
,
Lin, L.
,
Hsieh, B.-C.
,
Sánchez, S.F.
,
Ibarra-Medel, H.
,
Boquien, M.
,
Lacerna, I.
,
Argudo-Fernández, M.
,
Bizyaev, D.
,
Cano-Díaz, M.
,
Drory, N.
,
Gao, Y.
,
Masters, K.
,
Pan, K.
,
Tabor, M.
,
Tissera, P.
,
Xiao, T.
,
[SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR-M ∗ Relations on Galaxy Properties]
,
SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR-M ∗ Relations on Galaxy Properties
