output
19992026
most citedFormation of asteroid pairs by rotational fission

214 citations

Showing 2007 · astro-phShow all

10 papers · 2 filters

astro-ph2007★ 96 cited

IPHAS and the symbiotic stars. I. Selection method and first discoveries

R. L. M. Corradi, E. R. Rodríguez-Flores, A. Mampaso +7

The study of symbiotic stars is essential to understand important aspects of stellar evolution in interacting binaries. Their observed population in the Galaxy is however poorly kn…

astro-ph2007★ 75 cited

A multispectral view of the periodic events in eta Carinae

A. Damineli, D. J. Hillier, M. F. Corcoran +13

A full description of the 5.5-yr low excitation events in Eta Carinae is presented. We show that they are not as simple and brief as previously thought, but a combination of two co…

astro-ph2007★ 2 cited

The dependence of the viscosity-parameter on the disk scale height profile

Cesar Meirelles Filho, Nelson Leister

It is shown that the height scale for accretion disks is a constant whenever hydrostatic equilibrium and sub-sonic turbulence regime hold in the disk. In order to have a variable h…

astro-ph2007★ 43 cited

Bayesian posterior classification of planetary nebulae according to the Peimbert types

C. Quireza, H. J. Rocha-Pinto, W. J. Maciel

In this paper we present a re-analysis of the criteria used to characterize the Peimbert classes I, IIa, IIb, III and IV, through a statistical study of a large sample of planetary…

astro-ph2007★ 16 cited

Ages of Elliptical Galaxies: Single versus Multi Population Interpretation

T. P. Idiart, J. Silk, J. A. de Freitas Pacheco

New calibrations of spectrophotometric indices of elliptical galaxies as functions of spectrophotometric indices are presented, permitting estimates of mean stellar population ages…

astro-ph2007★ 35 cited

Chemical evolution of the Small Magellanic Cloud based on planetary nebulae

T. P. Idiart, W. J. Maciel, R. D. D. Costa

We investigate the chemical evolution of the Small Magellanic Cloud (SMC) based on abundance data of planetary nebulae (PNe). The main goal is to investigate the time evolution of…