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20032007
most citedThe K luminosity-metallicity relation for dwarf galaxies and the tidal dwarf galaxies in the tails of HCG 31

41 citations · 72 across the 3 of their papers we have counts for

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6 papers

astro-ph200731 cited

Seyfert's Sextet: A Slowly Dissolving Stephan's Quintet?

A. Durbala, A. del Olmo, M. S. Yun +7

We present a multiwavelength study of the highly evolved compact galaxy group known as Seyfert's Sextet (HCG79: SS). We interpret SS as a 2-3 Gyr more evolved analog of Stephan's Q…

astro-ph2006

From Nearby to High Redshift Compact Group of Galaxies

Philippe Amram, Chantal Balkowski, Claudia Mendes de Oliveira +2

Nearby Compact Groups of Galaxies (CGs) are very complex systems, tracing their history is a challenge (e.g. Stephan's Quintet). The presence of a diffuse X-rays emission that ofte…

astro-ph200641 cited

The K luminosity-metallicity relation for dwarf galaxies and the tidal dwarf galaxies in the tails of HCG 31

Claudia L. Mendes de Oliveira, Sonia Temporin, Eduardo S. Cypriano +4

We determine a K-band luminosity-metallicity (K-Z) relation for dwarf irregular galaxies, over a large range of magnitudes, -20.5 < M_K < -13.5, using a combination of K photometry…

astro-ph2005

GMOS-IFU Spectroscopy of 167-317 (LV2) Proplyd in Orion

M. J. Vasconcelos, A. H. Cerqueira, H. Plana +2

We present high spatial resolution spectroscopic observations of the proplyd 167-317 (LV2) near the Trapezium cluster in the Orion nebula, obtained during the System Verification r…

astro-ph2004

The Compact Group of Galaxies HCG 31 is in an early phase of merging

P. Amram, C. Mendes de Oliveira, H. Plana +1

We have obtained high spectral resolution (R = 45900) Fabry-Perot velocity maps of the Hickson Compact Group HCG 31 in order to revisit the important problem of the merger nature o…

astro-ph2003

Dynamical effects of interactions and the Tully-Fisher relation for Hickson compact groups

C. Mendes de Oliveira, P. Amram, H. Plana +1

We investigate the properties of the B-band Tully-Fisher (T-F) relation for 25 compact group galaxies, using Vmax derived from 2-D velocity maps. Our main result is that the majori…