| Publication |
Physical conditions in the gas phases of the giant H II region LMC-N 11 unveiled by Herschel . I. Diffuse [C II] and [O III] emission in LMC-N 11B, Lebouteiller, V.,Cormier, D.,Madden, S. C., Astronomy and Astrophysics, 548, 2012-12-01 00:00:00, 2012A&A...548A..91L||Pre-main-sequence stars in the stellar association N 11 in the Large Magellanic Cloud: clustering properties, Vallenari, Antonella,Sordo, Rosanna,Chiosi, Emanuela, Star Clusters: Basic Galactic Building Blocks Throughout Time and Space, 266, 2010-01-01 00:00:00, 2010IAUS..266..545V||Pre-main sequence stars in the stellar association N11 in the Large Magellanic Cloud, Vallenari, A.,Chiosi, E.,Sordo, R., Astronomy and Astrophysics, 511, 2010-02-01 00:00:00, 2010A&A...511A..79V||The effects of star formation on the low-metallicity ISM: NGC 4214 mapped with Herschel/PACS spectroscopy, Cormier, D.,Madden, S. C.,Hony, S., Astronomy and Astrophysics, 518, 2010-07-01 00:00:00, 2010A&A...518L..57C||The Young Stellar Population of NGC 4214 as Observed with the Hubble Space Telescope. I. Data and Methods, Úbeda, Leonardo,Apellániz, Jesús Maíz,MacKenty, John W., The Astronomical Journal, 133, 2007-03-01 00:00:00, 2007AJ....133..917U||The Young Stellar Population of NGC 4214 as Observed with the Hubble Space Telescope. II. Results, Úbeda, Leonardo,Apellániz, Jesús Maíz,MacKenty, John W., The Astronomical Journal, 133, 2007-03-01 00:00:00, 2007AJ....133..932U |
