Issue |
A&A
Volume 572, December 2014
|
|
---|---|---|
Article Number | A89 | |
Number of page(s) | 6 | |
Section | Catalogs and data | |
DOI | https://doi.org/10.1051/0004-6361/201424629 | |
Published online | 02 December 2014 |
Research Note
Young stellar object candidates toward the Orion region selected from GALEX⋆
S. D. Astronomía y Geodesia, Fac. CC. Matemáticas, Universidad Complutense
de Madrid,
28040
Madrid,
Spain
e-mail: nestorsa@ucm.es
Received:
18
July
2014
Accepted:
28
October
2014
We analyze 359 ultraviolet tiles from the All Sky Imaging Survey of the space mission GALEX covering roughly 400 square degrees toward the Orion star-forming region. There are a total of 1 555 174 ultraviolet sources that were cross-matched with other catalogs (2MASS, UCAC4, SDSS, DENIS, CMC15, and WISE) to produce a list of 290 717 reliable sources with a wide range of photometric information. Using different color selection criteria, we identify 111 young stellar object candidates showing both ultraviolet and infrared excesses, of which 81 are new identifications. We discuss the spatial distribution, the spectral energy distributions, and other physical properties of these stars. Their properties are, in general, compatible with those expected for T Tauri stars. This population of TTS candidates is widely dispersed around the Orion molecular cloud.
Key words: stars: low-mass / stars: pre-main sequence / stars: variables: T Tauri, Herbig Ae/Be / ultraviolet: stars
Full Tables 1 and 2 are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/572/A89
© ESO, 2014
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.