Browsing by Author "Israel, F."

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, 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 ...
    • Erratum: “The Herschel inventory of the agents of galaxy evolution (Heritage) in The Magellanic Clouds, a ... 
      Meixner, M.; Panuzzo, P.; Roman Duval, Julia; 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)
    • Millimeter dust emission compared with other mass estimates in N11 molecular clouds in the LMC 
      Herrera, C.; Rubio López, Mónica; Bolatto, A.; Boulanger, F.; Israel, F.; Rantakyro, F. (EDP Sciences, 2013)
      CO and dust emission at millimeter wavelengths are independent tracers of cold interstellar matter, which have seldom been compared on the scale of giant molecular clouds (GMCs) in other galaxies. In this study, and for ...
    • The State-of-Play of Anomalous Microwave Emission (AME) research 
      Dickinson, Clive; Ali-Haïmoud, Y.; Barr, A.; Battistelli, E.; Bell, A.; Bernstein, L.; Casassus Montero, Simón; Cleary, K.; Draine, B.; Génova-Santos, R.; Harper, S.; Hensley, B.; Hill-Valler, J.; Hoang, Thiem; Israel, F.; Jew, L.; Lazarian, A.; Leahy, J.; Leech, J.; López-Caraballo, C.; McDonald, I.; Murphy, E.; Onaka, T.; Paladini, R.; Peel, M.; Perrott, Y.; Poidevin, F.; Readhead, A.; Rubiño-Martín, J.; Taylor, A.; Tibbs, C.; Todorović, M.; Vidal, Matías (Elsevier B.V., 2018)
      Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997. ...
    • 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, 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 ...