Autor:
Riffel, Rogemar A.
Ho, Luis
Mason, Rachel
Rodríguez Ardila, Alberto
Martins, Lucimara
Riffel, Rogerio
Diaz, Ruben
Colina, Luis
Alonso-Herrero, Almudena
Flohic, Helene
González, Omaira
Lira Teillery, Paulina
McDermid, Richard
Ramos Almeida, Cristina
Schiavon, Ricardo
Thanjavur, Karun
Ruschel-Dutra, Daniel
Winge, Claudia
Perlman, Eric
Enlace original:
http://repositorio.uchile.cl/handle/2250/130657
Riffel, Rogemar A.
,
Ho, Luis
,
Mason, Rachel
,
Rodríguez Ardila, Alberto
,
Martins, Lucimara
,
Riffel, Rogerio
,
Diaz, Ruben
,
Colina, Luis
,
Alonso-Herrero, Almudena
,
Flohic, Helene
,
González, Omaira
,
Lira Teillery, Paulina
,
McDermid, Richard
,
Ramos Almeida, Cristina
,
Schiavon, Ricardo
,
Thanjavur, Karun
,
Ruschel-Dutra, Daniel
,
Winge, Claudia
,
Perlman, Eric
,
[Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?]