most citedNear-Infrared Spectroscopy of Carbon-Enhanced Metal-Poor Stars. I. A SOAR/OSIRIS Pilot Study

36 citations · 36 across the 2 of their papers we have counts for

collaborators

11 papers

astro-ph200866 cited

Hydrodynamical simulations of Galactic fountains I: evolution of single fountains

C. Melioli, F. Brighenti, A. D'Ercole +1

The ejection of the gas out of the disk in late-type galaxies is related to star formation and is due mainly to Type II supernovae. In this paper we studied in detail the developme…

astro-ph200636 cited

Near-Infrared Spectroscopy of Carbon-Enhanced Metal-Poor Stars. I. A SOAR/OSIRIS Pilot Study

Timothy C. Beers, Thirupathi Sivarani, Brian Marstellar +3

We report on an abundance analysis for a pilot study of seven Carbon-Enhanced Metal-Poor (CEMP) stars, based on medium-resolution optical and near-infrared spectroscopy. The optica…

astro-ph200617 cited

A Catalog of Candidate Field Horizontal-Branch and A-Type Stars. III. A 2MASS-Cleaned Version

Timothy C. Beers, Tiago Almeida, Silvia Rossi +2

We present coordinates and available photometric information (either from previous or recent broadband UBV observations, and near-infrared photometry from the 2MASS Point Source Ca…

astro-ph200616 cited

Dynamical evidence of the age--metallicity relation in the Milky Way disk

H. J. Rocha-Pinto, R. H. O. Rangel, G. F. Porto de Mello +2

We studied the relationship between the average stellar abundance of several elements and the orbital evolution of stars in the neighbourhood of the Sun, using both observational d…

astro-ph200610 cited

Optical polarimetric monitoring of the type II-plateau SN 2005af

A. Pereyra, A. M. Magalhaes, C. V. Rodrigues +4

Aims. Core-collapse supernovae may show significant polarization that implies non-spherically symmetric explosions. We observed the type II-plateau SN 2005af using optical polarime…

astro-ph2005

Polarimetry of Li-rich giants

A. Pereyra, B. V. Castilho, A. M. Magalhaes

Protoplanetary nebulae typically present non-spherical envelopes. The origin of such geometry is still controversial. There are indications that it may be carried over from an earl…