Now showing items 1-14 of 14

    • A 50 pc Scale View of Star Formation Efficiency across NGC 628 

      Kreckel, K.; Faesi, C.; Kruijssen, J. M. D.; Schruba, A.; Groves, B.; Leroy, A. K.; Bigiel, F.; Blanc, G. A.; Chevance, M.; Herrera C., Daniel; Hughes, A.; McElroy, R.; Pety, J.; Querejeta, M.; Rosolowsky, E.; Schinnerer, E.; Sun, J.; Usero, A.; Utomo, D. (Institute of Physics Publishing, 2018)
      © 2018. The American Astronomical Society. All rights reserved..Star formation is a multi-scale process that requires tracing cloud formation and stellar feedback within the local (≲kpc) and global galaxy environment. We ...
    • A 50 pc scale view of star formation efficiency across NGC 628 

      Kreckel, K.; Faesi, C.; Kruijssen, J. M. D.; Schruba, A.; Groves, B.; Leroy, A. K.; Bigiel, F.; Blanc, G. A.; Chevance, M.; Herrera C., Daniel; Hughes, A.; McElroy, R.; Pety, J.; Querejeta, M.; Rosolowsky, E.; Schinnerer, E.; Sun, J.; Usero, A.; Utomo, D. (IOP Publishing, 2018-08-20)
      Star formation is a multi-scale process that requires tracing cloud formation and stellar feedback within the local (less than or similar to kpc) and global galaxy environment. We present first results from two large ...
    • A revised planetary nebula luminosity function distance to NGC 628 using muse 

      Kreckel, K.; Groves, B.; Bigiel, F.; Blanc, G. A.; Kruijssen, J. M.D.; Hughes, A.; Schruba, A.; Schinnerer, E. (IOP Publishing, 2017)
      Distance uncertainties plague our understanding of the physical scales relevant to the physics of star formation in extragalactic studies. The planetary nebulae luminosity function (PNLF) is one of very few techniques that ...
    • AGN feedback in the nucleus of M51 

      Querejeta, M.; Schinnerer, E.; García Burillo, S.; Bigiel, F.; Blanc Mendiberri, Guillermo; Colombo, D.; Hughes, A.; Kreckel, K.; Leroy, A. K.; Meidt, S. E.; Meier, D. S.; Pety, J.; Sliwa, K. (EDP Sciences, 2016)
      AGN feedback is invoked as one of the most relevant mechanisms that shape the evolution of galaxies. Our goal is to understand the interplay between AGN feedback and the interstellar medium in M 51, a nearby spiral galaxy ...
    • Characterizing spiral arm and interarm star formation 

      Kreckel, K.; Blanc Mendiberri, Guillermo; Schinnerer, E.; Groves, B.; Adamo, A.; Hughes, A.; Meidt, S. (2016)
      Interarm star formation contributes significantly to a galaxy's star formation budget and provides an opportunity to study stellar birthplaces unperturbed by spiral arm dynamics. Using optical integral field spectroscopy ...
    • CHARACTERIZING THE LOW-MASS MOLECULAR COMPONENT IN THE NORTHERN SMALL MAGELLANIC CLOUD 

      Muller, E.; Ott, Jürgen; Hughes, A.; Pineda, J. L.; Wong, T.; Mizuno, Norikazu; Kawamura, Akiko; Mizuno, Y.; Fukui, Yasuo; Onishi, T.; Rubio López, Mónica (2010-01-26)
      We present here the first results from a high-resolution survey of the 12CO(J=1-0) emission across the northern part of the poorly-enriched Small Magellanic Cloud, made with the ATNF Mopra telescope. Three molecular ...
    • 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 ...
    • 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 ...
    • 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 ...
    • 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)
    • 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 inventory of the agents of galaxy evolution in the magellanic clouds, a herschel open time key program 

      Meixner, M.; Panuzzo, P.; Roman Duval, J.; Engelbracht, C.; Babler, B.; Seale, J. P.; Hony, S.; Montiel, E.; Sauvage, M.; Gordon, K.; Misselt, K.; Okumura, K.; Chanial, P.; Beck, T.; Bernard, J. P.; Bolatto, A.; Bot, C.; Boyer, M. L.; Carlson, L. R.; Clayton, G. C.; Chen, C.-H. R.; Cormier, D.; Fukui, Y.; Galametz, M.; Galliano, F.; Hora, J. L.; Hughes, A.; Indebetouw, R.; Israel, F.P.; Kawamura, A.; Kemper, F.; Kim, S.; Kwon, E.; Lebouteiller, V.; Li, A.; Long, K. S.; Madden, S. C.; Matsuura, M.; Muller, E.; Oliveira, J. M.; Onishi, T.; Otsuka, M.; Paradis, D.; Poglitsch, A.; Reach, W. T.; Robitaille, T. P.; Rubio López, Mónica; Sargent, B.; Sewiłlo, M.; Skibba, R.; Smith, L.; Srinivasan, S.; Tielens, A.; van Loon, J. Th.; Whitney, B. (The American Astronomical Society, 2013)
      We present an overview of the HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) in the Magellanic Clouds project, which is a Herschel Space Observatory open time key program. We mapped the Large Magellanic ...
    • 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 ...