Autor:
Roman-Lopes, A.
Román-Zúñiga, C.
Tapia, M.
Chojnowski, D.
Gómez Maqueo Chew, Y.
García-Hernández, D.A.
Borissova, J.
Minniti, D.
Covey, K.R.
Longa-Peña, P.
Fernandez-Trincado, J.G.
Zamora, O.
Nitschelm, C.
In this work, we make use of DR14 APOGEE spectroscopic data to study a sample of 92 known OB stars. We developed a near-infrared semi-empirical spectral classification method that was successfully used in case of four new exemplars, previously classified as later B-type stars. Our results agree w...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/7045
Roman-Lopes, A.
,
Román-Zúñiga, C.
,
Tapia, M.
,
Chojnowski, D.
,
Gómez Maqueo Chew, Y.
,
García-Hernández, D.A.
,
Borissova, J.
,
Minniti, D.
,
Covey, K.R.
,
Longa-Peña, P.
,
Fernandez-Trincado, J.G.
,
Zamora, O.
,
Nitschelm, C.
,
[Massive stars in the SDSS-IV/APOGEE SURVEY. I. OB stars]
,
Massive stars in the SDSS-IV/APOGEE SURVEY. I. OB stars
