Browsing by Author "Tielens, A. G. G. M."

Now showing items 1-5 of 5

    • 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, Julia; 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 ...
    • HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE): The Large Magellanic Cloud dust 
      Meixner, M.; Galliano, F.; Hony, S.; Roman Duval, Julia; 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 30 doradus molecular cloud at 0.4 pc resolution with the Atacama large millimeter/submillimeter array: ... 
      Wong, Tony; Oudshoorn, Luuk; Sofovich, Eliyahu; Green, Alex; Shah, Charmi; Indebetouw, Rémy; Meixner, Margaret; Hacar, Alvaro; Nayak, Omnarayani; Tokuda, Kazuki; Bolatto, Alberto D.; Chevance, Mélanie; De Marchi, Guido; Fukui, Yasuo; Hirschauer, Alec S.; Jameson, K. E.; Kalari, Venu; Lebouteiller, Vianney; Looney, Leslie W.; Madden, Suzanne C.; Onishi, Toshikazu; Román Duval, Julia; Rubio López, Mónica Solange; Tielens, A. G. G. M. (IOP, 2022)
      We present results of a wide-field (approximately 60 x 90 pc) Atacama Large Millimeter/submillimeter Array mosaic of CO(2-1) and (CO)-C-13(2-1) emission from the molecular cloud associated with the 30 Doradus star-forming ...
    • THE SPITZER SPECTROSCOPIC SURVEY OF THE SMALL MAGELLANIC CLOUD ((SMC)-M-4): PROBING THE PHYSICAL STATE OF ... 
      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 ...