activity
19972017
most citedThe Chemical Enrichment History of the Small Magellanic Cloud and Its Gradients

139 citations · 362 across the 10 of their papers we have counts for

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astro-ph2008★ 139 cited

The Chemical Enrichment History of the Small Magellanic Cloud and Its Gradients

Ricardo Carrera, Carme Gallart, Antonio Aparicio +3

We present stellar metallicities derived from Ca II triplet spectroscopy in over 350 red giant branch stars in 13 fields distributed in different positions in the SMC, ranging from…

astro-ph2005★ 17 cited

Three active M dwarfs within 8 pc: L 449-1, L 43-72, & LP 949-15

R. -D. Scholz, G. Lo Curto, R. A. Méndez +4

Three nearby star candidates were selected as bright 2MASS point sources without associated optical sources, i.e. with potentially large proper motions, subsequently confirmed by m…

astro-ph2004

Searching for White and Brown Dwarfs in the frame of the MUSYC/CYDER survey

M. Altmann, R. A. M'endez, M. -T. Ruiz +4

MUSYC (MUltiwavelength Survey by Yale and Chile), and its predecessor, the CYDER (Cal'an Yale Deep Extragalactic Research) survey are both deep multiwavelength surveys mainly aimin…

astro-ph1999★ 47 cited

Faint blue objects on the Hubble Deep Field North & South as possible nearby old halo white dwarfs

R. A. Méndez, D. Minniti

Using data derived from the deepest and finest angular resolution images of the universe yet acquired by astronomers at optical wavelengths using the Hubble Space Telescope (HST) i…

astro-ph1999★ 32 cited

A large local rotational speed for the Galaxy found from proper-motions: Implications for the mass of the Milky-Way

René A. Méndez, Imants Platais, Terrence M. Girard +2

Predictions from a Galactic Structure and Kinematic model are compared to the absolute proper-motions of about 30,000 randomly selected stars with derived fr…

astro-ph1997★ 1 cited

A new optical reddening model for the Solar neighborhood: Galactic Structure through low-latitude starcounts from the Guide Star Catalogue

R. A. Mendez, W. F. van Altena

A new optical reddening model for the Solar neighborhood is presented. The model makes use of the large-scale properties of the dust layer in the Galaxy, and of the observed clumpi…