Now showing items 1-6 of 6

    • 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 Emission at 8 and 24 µm as Diagnostics of H II Region Radiative Transfer 

      Oey, M. S.; López Hernández, J.; Kellar, J. A.; Pellegrini, E. W.; Gordon, K. D.; Jameson, K. E.; Li, A.; Madden, S. C.; Meixner, M.; Roman Duval, J.; Bot, C.; Rubio López, Mónica; Tielens, A. G. G. M. (IOP Publishing Ltd, 2017)
      We use the Spitzer Surveying the Agents of Galaxy Evolution (SAGE) survey of the Magellanic Clouds to evaluate the relationship between the 8 mu m polycyclic aromatic hydrocarbon (PAH) emission, 24 mu m hot dust emission, ...
    • 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 SPITZER SPECTROSCOPIC SURVEY OF THE SMALL MAGELLANIC CLOUD ((SMC)-M-4): PROBING THE PHYSICAL STATE OF POLYCYCLIC AROMATIC HYDROCARBONS IN A LOW-METALLICITY ENVIRONMENT 

      Sandstrom, Karin M.; Bolatto, Alberto; Bot, Caroline; Draine, B. T.; Ingalls, James G.; Israel, Frank P.; Jackson, James M.; Leroy, Adam K.; Li, Aigen; Rubio López, Mónica; Simon, Joshua D.; Smith, J. D. T.; Stanimirovic, Snezana; Tielens, A. G. G. M.; Loon, Jacco Th. van (IOP PUBLISHING LTD, 2012-01-01)
      We present results of mid-infrared spectroscopic mapping observations of six star-forming regions in the Small Magellanic Cloud (SMC) from the Spitzer Spectroscopic Survey of the SMC ((SMC)-M-4). We detect the mid-IR ...
    • Very Large Telescope observations of Gomez's Hamburger: Insights into a young protoplanet candidate 

      Berné, O.; Fuente, A.; Pantin, E.; Bujarrabal, V.; Baruteau, C.; Pilleri, P.; Habart, E.; Ménard, Francois; Cernicharo, J.; Tielens, A. G. G. M.; Joblin, C. (ESO, 2015)
      Planets are thought to form in the gas and dust disks around young stars. In particular, it has been proposed that giant planets can form through the gravitational instability of massive extended disks around intermediate-mass ...