Browsing by Author "XX564628"

Now showing items 21-36 of 36

    • The relationship between CO emission and visual extinction traced by dust emission in the Magellanic Clouds 
      Lee, Cheoljong; Leroy, Adam K.; Schnee, Scott; Wong, Tony; Bolatto, Alberto D.; Indebetouw, Remy; Rubio López, Mónica (Royal Astronomical Society, 2015)
      To test the theoretical understanding that finding bright CO emission depends primarily on dust shielding, we investigate the relationship between CO emission (I-CO) and the amount of dust (estimated from infrared emission ...
    • Results of the ESO-SEST key programme: CO in the Magellanic Clouds VI. The 30 Doradus Complex 
      Kutner, M. L.; Rubio López, Mónica; Booth, Roy S.; Boulanger, Francois; Graauw, Th. de; Garay Brignardello, Guido; Israel, F.P.; Johansson, L.E.B.; Lequeux, J.; Nyman, L. A. (Editions Physique, 1997-04)
      We report observations of 12CO(1 ! 0) emission from molecular clouds in a complex extending 2 kpc south of 30 Dor in the Large Magellanic Cloud. The observations were taken on the Swedish-ESO Submillimetre Telescope ...
    • Results of the ESO-SEST Key Programme: CO in the Magellanic Clouds. V. Further CO observations of the Small ... 
      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 southern molecular environment of SNR G18.8+0.3 (Research Note) 
      Paron, S.; Celis Peña, M.; Ortega, M. E.; Petriella, A.; Rubio López, Mónica; Dubner, G.; Giacani, E. (EDP Sciences, 2015)
      Aims. In a previous paper we investigated the molecular environment toward the eastern border of the supernova remnant (SNR) G18.8+0.3. Continuing with the study of the surroundings of this SNR, we now focus on its southern ...
    • 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, Julia; 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 ...
    • Star forming regions linked to RCW78 and the discovery of a new IR bubble 
      Cappa, C. E.; Rubio López, Mónica; Romero, G. A.; Duronea, N. U.; Firpo, V. (ESO, 2014)
      Aims. With the aim of investigating the presence of molecular and dust clumps linked to two star forming regions identified in the expanding molecular envelope of the stellar wind bubble RCW78, we analyzed the distribution ...
    • Study of a bright-rimmed cloud at the border of the infrared dust bubble CN20 
      Ortega, M. E.; Giacani, E.; Paron, S.; Rubio López, Mónica (Oxford Univ Press, 2016)
      We characterize an uncatalogued bright-rimmed cloud located at the border of the infrared dust bubble CN20 with the aim of investigating triggered star formation. In order to do this, we carried out radio continuum ...
    • Study of the molecular and ionized gas in a possible precursor of an ultra-compact HII region 
      Ortega, M. E.; Paron, S.; Giacani, E.; Celis Pena, M.; Rubio López, Mónica; Petriella, A. (EDP Sciences, 2017)
      Aims. We aim to study the molecular and the ionized gas in a possible precursor of an ultra-compact H II region to contribute to the understanding of how high-mass stars build-up their masses once they have reached the ...
    • Study of the molecular clump associated with the high-energy source HESS J1858+020 
      Paron, S.; Giacani, E.; Rubio López, Mónica; Dubner, G. (2011)
      Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A molecular cloud, composed of two clumps, shows signs of interaction with both the SNR and a nearby extended HII region. ...
    • Studying star-forming processes at core and clump scales: the case of the young stellar object G29.862-0.0044 
      Areal, M. B.; Paron, S.; Fariña, C.; Ortega, M. E.; Celis Peña, M.; Rubio López, Mónica (EDP Science, 2020)
      Aims. To advance our knowledge of star formation, in addition to statistical studies and large surveys of young stellar objects (YSOs), it is important to carry out detailed studies towards particular objects. Given that ...
    • Submillimeter studies of cold gas and dust in the Magellanic Clouds 
      Verdugo Salgado, Celia Anahi (Universidad de Chile, 2012)
      Presentamos datos a 870 mu obtenidos con el telescopio APEX en la SMC, LMC y puente Magallanico, obteniendo imagenes con 22 .4'' de resolucion para 9 nubes moleculares gigantes. Usamos estos datos en combinacion con ...
    • The magellanic bridge cluster NGC 796: deep optical AO imaging reveals the stellar content and initial mass ... 
      Kalari, Venu M.; Carraro, Giovanni; Evans, Christopher J.; Rubio López, Mónica (IOP Publishing Ltd, 2018)
      NGC 796 is a massive young cluster located 59 kpc from us in the diffuse intergalactic medium of the 1/5-1/10 Z(circle dot) Magellanic Bridge, allowing us to probe variations in star formation and stellar evolution processes ...
    • The molecular environment of the pillar like features in the H II region G46.5–0.2 
      Paron, S.; Celis Peña, M.; Ortega, M. E.; Fariña, C.; Petriella, A.; Rubio López, Mónica; Ashley, R. P. (Oxford University Press, 2017)
      At the interface of H II regions and molecular gas, peculiar structures appear, some of them with pillar-like shapes. Understanding their origin is important for characterizing triggered star formation and the impact of ...
    • The Relationship Between Molecular GAS, H I, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds 
      Jameson, Katherine E.; Bolatto, Alberto D.; Leroy, Adam K.; Meixner, Margaret; Roman Duval, Julia; Gordon, Karl D.; Hughes, Annie; Israel, Frank P.; Rubio López, Mónica; Indebetouw, Remy; Madden., Suzanne C.; Bot, Caroline; Hony, Sach; Cormier, Diane; Pellegrini, Eric W.; Galametz, Maud; Sonneborn, George (2016)
      The Magellanic Clouds provide the only laboratory to study the effects of metallicity and galaxy mass on molecular gas and star formation at high (similar to 20 pc) resolution. We use the dust emission from HERITAGE Herschel ...
    • A view of Large Magellanic Cloud H II regions N159, N132, and N166 through the 345-GHz window 
      Paron, S.; Ortega, M. E.; Fariña, C.; Cunningham, M.; Jones, P. A.; Rubio López, Mónica (Oxford University Press, 2016)
      We present results obtained towards the H II regions N159, N166, and N132 from the emission of several molecular lines in the 345 GHz window. Using Atacama Submillimetre Telescope Experiment, we mapped a 2.4 arcmin x 2.4 ...