Autor:
Gonzalez, O.A.
Gadotti, D.A.
Debattista, V.P.
Rejkuba, M.de
Valenti, E.
Zoccali, M.
Coccato, L.
Minniti, D.
Ness, M.
Context. Our view of the structure of the Milky Way and, in particular, its bulge is obscured by the intervening stars, dust, and gas in the disc. While great progress in understanding the bulge has been achieved with past and ongoing observations, the comparison of its global chemodynamical prop...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/836
Gonzalez, O.A.
,
Gadotti, D.A.
,
Debattista, V.P.
,
Rejkuba, M.de
,
Valenti, E.
,
Zoccali, M.
,
Coccato, L.
,
Minniti, D.
,
Ness, M.
,
[Comparing the properties of the X-shaped bulges of NGC 4710 and the Milky Way with MUSE]
,
Comparing the properties of the X-shaped bulges of NGC 4710 and the Milky Way with MUSE
