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Title:
The ionized gas in and around the Wolf-Rayet galaxy NGC 1741
Authors:
López-Sánchez, Ángel R.; Esteban, César; Rodríguez, Mónica
Affiliation:
AA(Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, E-38200 La Laguna, Tenerife, España), AB(Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, E-38200 La Laguna, Tenerife, España), AC(Instituto Nacional de Astronomía, Óptica y Electrónica, Apdo. Postal 51 y 216, 72000 Puebla, Pue., México)
Publication:
A Massive Star Odyssey: From Main Sequence to Supernova, Proceedings of IAU Symposium #212, held 24-28 June 2001 in Lanzarote, Canary island, Spain. Edited by Karel van der Hucht, Artemio Herrero, and Esteban, César. San Francisco: Astronomical Society of the Pacific, 2003., p.728
Publication Date:
00/2003
Origin:
AUTHOR
Bibliographic Code:
2003IAUS..212..728L

Abstract

Interaction can be the main mechanism that triggers star formation in Wolf-Rayet galaxies. The compact group HCG 31 has one of this objects, NGC 1741. We present new observations of this compact interacting group, in order to analyse the physical conditions and chemical composition of the ionized gas, as well as to estimate the ages of the starbursts.

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