Now showing items 1-5 of 5

    • The dust properties and physical conditions of the interstellar medium in the LMC massive star-forming complex N11 

      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, J.; 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 ...
    • Erratum: “The Herschel inventory of the agents of galaxy evolution (Heritage) in The Magellanic Clouds, a Herschel Open Time Key Program” (2013, aj, 146, 62) 

      Meixner, M.; Panuzzo, P.; Roman Duval, J.; Engelbracht, C.; Babler, B.; Seale, J.; Hony, S.; Montiel, E.; Sauvage, M.; Gordon, K.; Misselt, K.; Okumura, K.; Chanial, P.; Beck, T.; Bernard, J.; Bolatto, A.; Bot, C.; Boyer, M.; Carlson, L.; Clayton, G.; Chen, C.; Cormier, D.; Fukui, Y.; Galametz, M.; Galliano, F.; Hora, J.; Hughes, A.; Indebetouw, R.; Israel, F.; Kawamura, A.; Kemper, F.; Kim, S.; Kwon, E.; Lebouteiller, V.; Li, A.; Long, K.; Madden, S.; Matsuura, M.; Muller, E.; Oliveira, J.; Onishi, T.; Otsuka, M.; Paradis, D.; Poglitsch, A.; Reach, W.; Robitaille, T.; Rubio López, Mónica; Sargent, B.; Sewilo, M.; Skibba, R.; Smith, L.; Srinivasan, S.; Tielens, A.; van Loon, J.; Whitney, B. (IOP PUBLISHING, 2015)
    • Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC 

      Hony, S.; Gouliermis, D.; Galliano, F.; Galametz, M.; Cormier, D.; Chen, C.; Dib, S.; Hughes, A.; Klessen, R.; Roman Duval, J.; Smith, L.; Bernard, J.; Bot, C.; Carlson, L.; Gordon, K.; Indebetouw, R.; Lebouteiller, V.; Lee, M.; Madden, S.; Meixner, M.; Oliveira, J.; Rubio López, Mónica; Sauvage, M.; Wu, R. (Oxford Univ Press, 2015)
      The rate at which interstellar gas is converted into stars, and its dependence on environment, is one of the pillars on which our understanding of the visible Universe is build. We present a comparison of the surface density ...
    • The Herschel Virgo Cluster Survey – VIII. The Bright Galaxy Sample 

      Davies, J. I.; Bianchi, S.; Cortese, L.; Auld, R.; Baes, Maarten; Bendo, G. J.; Boselli, A.; Ciesla, L.; Clemens, M.; Corbelli, E.; De Looze, I.; Alighieri, S. di Serego; Fritz, J.; Gavazzi, G.; Pappalardo, C.; Grossi, M.; Hunt, L. K.; Madden, S.; Magrini, L.; Pohlen, M.; Smith, M. W. L.; Verstappen, J.; Vlahakis, C. (2012)
      We describe the Herschel Virgo Cluster Survey and the first data that cover the complete survey area (four 4 × 4 deg2 regions). We use these data to measure and compare the global far-infrared properties of 78 optically ...
    • The thermal dust emission in N158–N159–N160 (LMC) star-forming complex mapped by Spitzer, Herschel and LABOCA 

      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, J.; Rubio López, Mónica; Sauvage, M.; Seale, J. P.; Sewiło, M.; van Loon, Th. (Royal Astronomical Society, 2013-03-08)
      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 ...