Now showing items 1-10 of 10

    • Cold dust clumps in dynamically hot gas 

      Kim, S.; Kwon, E.; Madden, S. C.; Meixner, M.; Hony, S.; Panuzzo, P.; Sauvage, M.; Roman-Duval, J.; Gordon, K. D.; Engelbracht, C.; Israel, F. P.; Misselt, K.; Okumura, K.; Li, A.; Bolatto, Alberto; Skibba, R.; Galliano, F.; Matsuura, M.; Bernard, J. P.; Bot, Caroline; Galametz, M.; Hughes, A.; Kawamura, A.; Onishi, T.; Paradis, D.; Poglitsch, A.; Reach, W. T.; Robitaille, T.; Rubio López, Mónica; Tielens, A. G. G. M. (EDP Sciences, 2010-07)
      Aims. We present clumps of dust emission from Herschel observations of the Large Magellanic Cloud (LMC) and their physical and statistical properties. We catalog cloud features seen in the dust emission from Herschel ...
    • Determining dust temperatures and masses in the Herschel era: The importance of observations longward of 200 micron 

      Gordon, K. D.; Galliano, F.; Hony, S.; Bernard, J. P.; Bolatto, Alberto; Bot, Caroline; Engelbracht, C.; Hughes, A.; Israel, F. P.; Kemper, F.; Kim, S.; Li, A.; Madden, S. C.; Matsuura, M.; Meixner, M.; Misselt, K.; Okumura, K.; Panuzzo, P.; Rubio López, Mónica; Reach, W. T.; Roman-Duval, J.; Sauvage, M.; Skibba, R.; Tielens, A. G. G. M. (ESO, 2010)
      The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (≥100 μm). Only with SPIRE on Herschel has it been possible to get high spatial resolution at 200 to 500 μm that is ...
    • Dust/gas correlations from Herschel observations 

      Roman Duval, J.; Israel, F. P.; Bolatto, Alberto; Hughes, A.; Leroy, A.; Meixner, M.; Gordon, K.; Madden, S. C.; Paradis, D.; Kawamura, A.; Li, A.; Sauvage, M.; Wong, T.; Bernard, J. P.; Engelbracht, C.; Hony, S.; Kim, S.; Misselt, K.; Okumura, K.; Ott, Jürgen; Panuzzo, P.; Pineda, J. L.; Reach, W. T.; Rubio López, Mónica (2010)
      12CO rotational emission lines and Hi 21 cm emission. This so-called “FIR excess” is especially noticeable near molecular clouds in the LMC, and has usually been interpreted as indicating the presence of a self-shielded ...
    • HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE): The Large Magellanic Cloud dust 

      Meixner, M.; Galliano, F.; Hony, S.; Roman-Duval, J.; Robitaille, T.; Panuzzo, P.; Sauvage, M.; Gordon, K.; Engelbracht, C.; Misselt, K.; Okumura, K.; Beck, T.; Bernard, J. P.; Bolatto, Alberto; Bot, Caroline; Boyer, M.; Bracker, S.; Carlson, L. R.; Clayton, G. C.; Chen, C.-H. R.; Churchwell, E.; Fukui, Y.; Galametz, M.; Hora, J. L.; Hughes, A.; Indebetouw, R.; Israel, F. P.; Kawamura, A.; Kemper, F.; Kim, S.; Kwon, E.; Lawton, B.; Li, A.; Long, K. S.; Marengo, M.; Madden, S. C.; Matsuura, M.; Oliveira, J. M.; Onishi, T.; Otsuka, M.; Paradis, D.; Poglitsch, A.; Riebel, D.; Reach, W. T.; Rubio López, Mónica; Sargent, B.; Sewiło, M.; Simon, J. D.; Skibba, R.; Smith, L. J.; Srinivasan, S.; Tielens, A. G. G. M.; van Loon, J. Th.; Whitney, B.; Woods, P. M. (EDP SCIENCES S A., 2010-07)
      The HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) of the Magellanic Clouds will use dust emission to investigate the life cycle of matter in both the Large and Small Magellanic Clouds (LMC and SMC). Using ...
    • The Herschel revolution: Unveiling the morphology of the high-mass star-formation sites N44 and N63 in the LMC 

      Hony, S.; Galliano, F.; Madden, S. C.; Panuzzo, P.; Meixner, M.; Engelbracht, C.; Misselt, K.; Galametz, M.; Sauvage, M.; Roman-Duval, J.; Gordon, K.; Lawton, B.; Bernard, J. P.; Bolatto, Alberto; Okumura, K.; Chen, C.-H. R.; Indebetouw, R.; Israel, F. P.; Kwon, E.; Li, A.; Kemper, F.; Oey, M. S.; Rubio López, Mónica; Triou, H. E. (EDP Sciences, 2010-07)
      Aims. We study the structure of the medium surrounding sites of high-mass star formation to determine the interrelation between the H ii regions and the environment from which they were formed. The density distribution of ...
    • Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds - IX - The giant LMC HII region complex N 11 

      Israel, F. P.; Graauw, Th. de; Johansson, L.E.B.; Booth, Roy S.; Boulanger, Francois; Garay Brignardello, Guido; Kutner, M. L.; Lequeux, J.; Nyman, L. A.; Rubio López, Mónica (EDP Sciences, 2003)
      The second-brightest star formation complex in the Large Magellanic Cloud, N 11, was surveyed extensively in the J = 1–0 transition of 12CO. In this paper we present maps and a catalogue containing the parameters of 29 ...
    • Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds X. CO emission from star formation regions in LMC and SMC 

      Israel, F. P.; Johansson, L.E.B.; Rubio López, Mónica; Garay Brignardello, Guido; Graauw, Th. de; Booth, Roy S.; Boulanger, Francois; Kutner, M. L.; Lequeux, J.; Nyman, L.-A. (EDP Sciences, 2003-08)
      We present J = 1−0 and J = 2−1 12CO maps of several star-forming regions in both the Large and the Small Magellanic Cloud, and briefly discuss their structure. Many of the detected molecular clouds are relatively isolated ...
    • Results of the ESO-SEST Key Programme: CO in the Magellanic Clouds. V. Further CO observations of the Small Magellanic Cloud 

      Rubio López, Mónica; Lequeux, J.; Boulanger, Francois; Booth, Roy S.; Garay Brignardello, Guido; de Graauw, Th.; Israel, F. P.; Johansson, L.E.B.; Kutner, M.L.; Nyman, L. A. (1996-08)
      We present further results of fully-sampled observations in the J = 1!0 and J = 2!1 rotational transitions of 12CO and 13CO, obtained with the SEST telescope at 43 00 or 22 00 resolution, toward the Small Magellanic Cloud. ...
    • Results of the SEST Key Programme: CO in the Magellanic Clouds VIII. The giant molecular complex No. 37 of the LMC 

      Garay Brignardello, Guido; Johansson, L. E. B.; Nyman, L. A.; Booth, Roy S.; Israel, F. P.; Kutner, M. L.; Lequeux, J.; Rubio López, Mónica (2002)
      We report observations of the CO(1!0), CO(2!1) and 13CO(1!0) line emission from the giant molecular complex No. 37 of the Large Magellanic Cloud, made with linear resolutions between 6 and 12 pc. The observations were ...
    • 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. C.; Albrecht, M.; Bot, Caroline; Cormier, D.; Engelbracht, C.; Fukui, Y.; Israel, F. P.; 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.; Loon, J. Th. van (Oxford University Press on behalf of the 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 ...