Now showing items 1-3 of 3

    • Galametz, M.; Hony, S.; Albrecht, M.; Galliano, F.; Cormier, D.; Lebouteiller, V.; Lee, M.; Madden, S.; Bolatto, A.; Bot, C.; Hughes, A.; Israel, F.; Meixner, M.; Oliviera, J.; Paradis, D.; Pellegrini, E.; Roman Duval, Julia; Rubio López, Mónica; Sewilo, M.; Fukui, Y.; Kawamura, A.; Onishi, T. (OXFORD UNIV PRESS, 2016)
      We combine Spitzer and Herschel data of the star-forming region N11 in the Large Magellanic Cloud (LMC) to produce detailed maps of the dust properties in the complex and study their variations with the interstellar-medium ...
    • Bot, Caroline; Rubio López, Mónica; Boulanger, Francois; Albrecht, M.; Leroy, A.; Bolatto, Alberto; Bertoldi, F.; Gordon, K.; Engelbracht, C.; Block, M.; Misselt, K. (2010)
      Context. The amount of molecular gas is a key to understanding the future star formation in a galaxy. Because H2 is difficult to observe directly in dense and cold clouds, tracers such as the CO molecule are used. However, ...
    • Galametz, M.; Hony, S.; Galliano, F.; Madden, S.; Albrecht, M.; Bot, C.; Cormier, D.; Engelbracht, C.; Fukui, Y.; Israel, F.; Kawamura, A.; Lebouteiller, V.; Li, A.; Meixner, M.; Misselt, K.; Montiel, E.; Okumura, K.; Panuzzo, P.; Roman Duval, Julia; Rubio López, Mónica; Sauvage, M.; Seale, J. P.; Sewiło, M.; Van Loon, Th. (Royal Astronomical Society, 2013)
      Low-metallicity galaxies exhibit different properties of the interstellar medium (ISM) compared to nearby spiral galaxies. Obtaining a resolved inventory of the various gas and dust components of massive star-forming ...