The ionized gas in and around the Wolf-Rayet galaxy NGC 1741

Bibcode
2003IAUS..212..728L
López-Sánchez, Ángel R.; Esteban, César; Rodríguez, Mónica
Referencia bibliográfica

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

Fecha de publicación:
0
2003
Número de autores
3
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro

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