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Article 2017-11

Autor: Minniti, D. Geisler, D. Alonso-Garcia, J. Palma, T. Beamin, J.C. Borissova, J. Catelan, M. Clariá, J.J. Cohen, R.E. Ramos, R.C. Dias, B. Fernández-Trincado, J.G. Gómez, M. Hempel, M. Ivanov, V.D. Kurtev, R. Lucas, P.W. Moni-Bidin, C. Pullen, J. Alegria, S.R. Saito, R.K. Valenti, E.

It is likely that a number of Galactic globular clusters remain to be discovered, especially toward the Galactic bulge. High stellar density combined with high and differential interstellar reddening are the two major problems for finding globular clusters located toward the bulge. We use the dee...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/5907

Repositorio Universidad Andrés Bello
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Minniti, D. ,  Geisler, D. ,  Alonso-Garcia, J. ,  Palma, T. ,  Beamin, J.C. ,  Borissova, J. ,  Catelan, M. ,  Clariá, J.J. ,  Cohen, R.E. ,  Ramos, R.C. ,  Dias, B. ,  Fernández-Trincado, J.G. ,  Gómez, M. ,  Hempel, M. ,  Ivanov, V.D. ,  Kurtev, R. ,  Lucas, P.W. ,  Moni-Bidin, C. ,  Pullen, J. ,  Alegria, S.R. ,  Saito, R.K. ,  Valenti, E. ,  [New VVV Survey Globular Cluster Candidates in the Milky Way Bulge] ,  New VVV Survey Globular Cluster Candidates in the Milky Way Bulge
Article 2016

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

Repositorio Universidad Andrés Bello
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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
Article 2016-03

Autor: Valenti, E. Zoccali, M. Gonzalez, O. A. Minniti, D. Alonso-García, J. Marchetti, E. Hempel, M. Renzini, A. Rejkuba, M.

We present the first stellar density profile of the Milky Way bulge that reaches latitude b = 0 degrees. The profile was derived by counting red clump stars within the colour-magnitude diagram that was constructed using the new PSF-fitting photometry from VISTA Variables in the Via Lactea (VVV) s...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/3974

Repositorio UNAB
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Valenti, E. ,  Zoccali, M. ,  Gonzalez, O. A. ,  Minniti, D. ,  Alonso-García, J. ,  Marchetti, E. ,  Hempel, M. ,  Renzini, A. ,  Rejkuba, M. ,  [Stellar density profile and mass of the Milky Way bulge from VVV data] ,  Stellar density profile and mass of the Milky Way bulge from VVV data

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