¡Nos trasladamos! E-Prints cerrará el 7 de junio.

En las próximas semanas vamos a migrar nuestro repositorio a una nueva plataforma con muchas funcionalidades nuevas. En esta migración las fechas clave del proceso son las siguientes:

Es muy importante que cualquier depósito se realice en E-Prints Complutense antes del 7 de junio. En caso de urgencia para realizar un depósito, se puede comunicar a docta@ucm.es.

Ultraviolet emission from stellar populations within tidal tails: Catching the youngest galaxies in formation?



Downloads per month over past year

Gil de Paz, Armando and otros, ... (2005) Ultraviolet emission from stellar populations within tidal tails: Catching the youngest galaxies in formation? Astrophysical journal, 619 (1). L91-L94. ISSN 0004-637X

[thumbnail of gildepaz123libre.pdf]

Official URL: http://dx.doi.org/10.1086/426137


New Galaxy Evolution Explorer (GALEX) observations have detected significant far-UV (FUV; 1530 Å) and near-UV (NUV; 2310 Å) emission from stellar substructures within the tidal tails of four ongoing galaxy mergers. The UV-bright regions are optically faint and are coincident with H I density enhancements. FUV emission is detected at any location where the H I surface density exceeds ~2 M_☉ pc^-2, and it is often detected in the absence of visible wavelength emission. UV luminosities of the brighter regions of the tidal tails imply masses of 10^6 to ~10^9 M_☉ in young stars in the tails, and H I luminosities imply similar H I masses. UV-optical colors of the tidal tails indicate stellar populations as young as a few megayears, and in all cases ages under 400 Myr. Most of the young stars in the tails formed in single bursts, rather than resulting from continuous star formation, and they formed in situ as the tails evolved. Star formation appears to be older near the parent galaxies and younger at increasing distances from the parent galaxy. This could be because the star formation occurs progressively along the tails, or because the star formation has been inhibited near the galaxy/tail interface. The youngest stellar concentrations, usually near the ends of long tidal tails, have masses comparable to confirmed tidal dwarf galaxies and may be newly forming galaxies undergoing their first burst of star formation.

Item Type:Article
Additional Information:

© 2005. The American Astronomical Society. All rights reserved. Artículo firmado por 25 autores. GALEX is a NASA small explorer launched in 2003 April. We gratefully acknowledge NASA’s support for construction, operation, and science analysis for the GALEX mission, developed in cooperation with the Centre National d’Etudes Spatiales of France and the Korean Ministry of Science and Technology.

Uncontrolled Keywords:Interacting galaxies; Merging galaxies; Dwarf galaxies; NGC-520; Gas
Subjects:Sciences > Physics > Astrophysics
Sciences > Physics > Astronomy
ID Code:36008
Deposited On:29 Feb 2016 16:05
Last Modified:10 Dec 2018 15:05

Origin of downloads

Repository Staff Only: item control page