YSOs in Camelopardalis (Straizys+, 2010)

Details YSOs in Camelopardalis (Straizys+, 2010) YSOs in Camelopardalis (Straizys+, 2010)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat.130190001s&link_type=abstract

VizieR On-line Data Catalog: J/BaltA/19/1. Originally published in: 2010BaltA..19....1S

Physics

Clusters: Open, Ysos, Cross Identifications

Scientific paper

Using photometric data of infrared surveys, young stellar object (YSO) status is verified for 141 objects selected in our previous papers in the Cassiopeia and Camelopardalis segment of the Milky Way bounded by Galactic Using photometric data of infrared surveys, young stellar object (YSO) status is verified for 141 objects selected in our previous papers in the Cassiopeia and Camelopardalis segment of the Milky Way bounded by Galactic (l, b) = 132-158°, +/-12°). The area includes the known starforming regions in the emission nebulae W3, W4 and W5 and the massive YSOAFGL 490. Spectral energy distribution (SED) curves between 700 nm and 160um, constructed from the GSC 2, 2MASS, IRAS, MSX, Spitzer and AKARI data, are used to estimate the evolutionary stages of these stars.
(1 data file).

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