Para depositar en Docta Complutense, identifícate con tu correo @ucm.es en el SSO institucional: Haz clic en el desplegable de INICIO DE SESIÓN situado en la parte superior derecha de la pantalla. Introduce tu correo electrónico y tu contraseña de la UCM y haz clic en el botón MI CUENTA UCM, no autenticación con contraseña.
 

Resolved stellar populations constituting extended UV disks (XUV-disks) in nearby galaxies

Thumbnail Image

Download

downoloadgildepaz90preprint.pdf (167.86 KB)

Official URL

http://adsabs.harvard.edu/abs/2007arXiv0712.3724T

Full text at PDC

Publication date

2008

Authors

Advisors (or tutors)

Editors

Journal Title

Journal ISSN

Volume Title

Publisher

Astronomical Society of the Pacific (ASP)
Citations
Google Scholar
Exportar
DC QDC MarcXML RDF MODS METS ORE-ATOM

URI

https://hdl.handle.net/20.500.14352/53489

Citation

Abstract

We describe HST imaging of recent star formation complexes located in the extended UV disk (XUV-disk) component of NGC 5236 (M 83), NGC 5055 (M 63), and NGC 2090. Photometry in four FUV-visible bands permits us to constrain the type of resolved stars and effective age of clusters, in addition to extinction. The preliminary results given herein focus on CMD analysis and clustering properties in this unique star-forming environment.

Research Projects

Organizational Units

Journal Issue

Description

© Astronomical Society of the Pacific (ASP). International Conference on Formation and Evolution of Galaxy Disks (2007. Rome, Italy). This work was supported by grants HST-GO-10608.01-A and HST-GO-10904.01-A.

UCM subjects

Astrofísica, Astronomía (Física)

Unesco subjects

Keywords

Collections

Secciones de libros