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Autor: Saito, R. K. Hempel, M. Minniti, D. Lucas, P. W. Rejkuba, M. Toledo, I. Gonzalez, O. A. Alonso-García, J. Irwin, M. Gonzalez-Solares, E. Hodgkin, S. T. Lewis, J. R. Cross, N. Ivanov, V. D. Kerins, E. Emerson, J. P. Soto, M. Amôres, E. B. Gurovich, S. Dékány, I. Angeloni, R. Beamin, J. C. Catelan, M. Padilla, N. Zoccali, M. Pietrukowicz, P. Moni Bidin, C. Mauro, F. Geisler, D. Folkes, S. L. Sale, S. E. Borissova, J. Kurtev, R. Ahumada, A. V. Alonso, M. V. Adamson, A. Arias, J. I. Bandyopadhyay, R. M. Barbá, R. H. Barbuy, B. Baume, G. L. Bedin, L. R. Bellini, A. Benjamin, R. Bica, E. Bonatto, C. Bronfman Aguiló, Leonardo Carraro, Giovanni Chenè, A. N. Clariá, J. J. Clarke, J. R. A. Contreras, C. Corvillón, A. Grijs, R. de Dias, B. Drew, J. E. Fariña, C. Feinstein, C. Fernández Lajús, E. Gamen, R. Gieren, W. Goldman, B. González-Fernández, C. Grand, R. J. J. Gunthardt, G. Hambly, N. C. Hanson, M. M. Helminiak, K. G. Hoare, M. G. Huckvale, L. Jordán, A. Kinemuch, K. Longmore, A. López Corredoira, M. Maccarone, T. Majaess, D. Martín, E. L. Masetti, N. Mennickent, R. E. Mirabel, I. F. Monaco, L. Morelli, L. Motta, V. Palma, T. Parisi, M. C. Parker, Q. Peñaloza, F. Pietrzynski, G. Pignata Libralato, Giuliano Popescu, B. Read, M. A. Rojas, A. Roman-Lopes, A. Ruiz González, María Teresa Saviane, I. Schreiber, M. R. Schröder, A. C. Sharma, S. Smith, M. D. Sodré Jr., L. Stead, J. Stephens, A. W. Tamura, M. Tappert, C. Thompson, M. A. Valenti, E. Vanzi, L. Walton, N. A. Weidmann, W. Zijlstr, A.

Saito, R. K.Hempel, M.Minniti, D.Lucas, P. W.Rejkuba, M.Toledo, I.Gonzalez, O. A.Alonso-García, J.Irwin, M.Gonzalez-Solares, E.Hodgkin, S. T.Lewis, J. R.Cross, N.Ivanov, V. D.Kerins, E.Emerson, J. P.Soto, M.Amôres, E. B.Gurovich, S.Dékány, I.Angeloni, R.Beamin, J. C.Catelan, M.Padilla, N.Zoccali, M.Pietrukowicz, P.Moni Bidin, C.Mauro, F.Geisler, D.Folkes, S. L.Sale, S. E.Borissova, J.Kurtev, R.Ahumada, A. V.Alonso, M. V.Adamson, A.Arias, J. I.Bandyopadhyay, R. M.Barbá, R. H.Barbuy, B.Baume, G. L.Bedin, L. R.Bellini, A.Benjamin, R.Bica, E.Bonatto, C.Bronfman Aguiló, LeonardoCarraro, GiovanniChenè, A. N.Clariá, J. J.Clarke, J. R. A.Contreras, C.Corvillón, A.Grijs, R. deDias, B.Drew, J. E.Fariña, C.Feinstein, C.Fernández Lajús, E.Gamen, R.Gieren, W.Goldman, B.González-Fernández, C.Grand, R. J. J.Gunthardt, G.Hambly, N. C.Hanson, M. M.Helminiak, K. G.Hoare, M. G.Huckvale, L.Jordán, A.Kinemuch, K.Longmore, A.López Corredoira, M.Maccarone, T.Majaess, D.Martín, E. L.Masetti, N.Mennickent, R. E.Mirabel, I. F.Monaco, L.Morelli, L.Motta, V.Palma, T.Parisi, M. C.Parker, Q.Peñaloza, F.Pietrzynski, G.Pignata Libralato, GiulianoPopescu, B.Read, M. A.Rojas, A.Roman-Lopes, A.Ruiz González, María TeresaSaviane, I.Schreiber, M. R.Schröder, A. C.Sharma, S.Smith, M. D.Sodré Jr., L.Stead, J.Stephens, A. W.Tamura, M.Tappert, C.Thompson, M. A.Valenti, E.Vanzi, L.Walton, N. A.Weidmann, W.Zijlstr, A.[VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Via Lactea]

Context. The globular cluster HP 1 is projected at only 3.̊33 from the Galactic center. Together with its distance, this makes it one of the most central globular clusters in the Milky Way. It has a blue horizontal branch (BHB) and a metallicity of [Fe/H] ≈ −1.0. This means that it probably is on...


Barbuy, B.Cantelli, E.Vemado, A.Ernandes, H.Ortolani, S.Saviane, I.Bica, E.Minniti, D.Dias, B.Momany, Y.Hill, V.Zoccali, M.Siqueira-Mello, C.[High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP 1]High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP 1

Context. Oxygen and zinc in the Galactic bulge are key elements for the understanding of the bulge chemical evolution. Oxygen-to-iron abundance ratios provide a most robust indicator of the star formation rate and chemical evolution of the bulge. Zinc is enhanced in metal-poor stars, behaving as ...


Da Silveira, C.R.Barbuy, B.Friaça, A.C.S.Hill, V.Zoccali, M.Rafelski, M.Gonzalez, O.A.Minniti, D.Renzini, A.Ortolani, S.[Oxygen and zinc abundances in 417 Galactic bulge red giants]Oxygen and zinc abundances in 417 Galactic bulge red giants

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