Browsing by Author "López Sepulcre, A."

Now showing items 1-3 of 3

    • ALMA-IMF III. Investigating the origin of stellar masses: top-heavy core mass function in the W43-MM2&MM3 ... 
      Pouteau, Y.; Motte, F.; Nony, T.; Galván Madrid, R.; Men’shchikov, A.; Bontemps, S.; Robitaille, J. F.; Louvet, Fabien; Ginsburg, A.; López Sepulcre, A.; Dell’Ova, P.; Gusdorf, A.; Sanhueza, P.; Stutz, Amelia Marie; Brouillet, N.; Thomasson, B.; Armante, M.; Baug, T.; Bonfand, M.; Busquet, G.; Csengeri, T.; Cunningham, N.; Fernández López, M.; Liu, H. L.; Olguin, F.; Towner, A. P. M.; Bally, J.; Braine, J.; Bronfman Aguiló, Leonardo Jaime; González, M.; Hennebelle, P.; Lu, X.; Menten, K. M.; Moraux, E.; Tatematsu, K.; Walker, D.; Whitworth, A. P. (EDP Sciences, 2021)
      Aims. The processes that determine the stellar initial mass function (IMF) and its origin are critical unsolved problems, with profound implications for many areas of astrophysics. The W43-MM2&MM3 mini-starburst ridge ...
    • H II regions and high-mass starless clump candidates: II. Fragmentation and induced star formation at similar ... 
      Zhang, S.; Zavagno, A.; López Sepulcre, A.; Liu, H.; Louvet, Fabien; Figueira, M.; Russeil, D.; Wu, Y.; Yuan, J.; Pillai, T. G. S (EDP Sciences, 2021)
      Context. The ionization feedback from H II regions modifies the properties of high-mass starless clumps (HMSCs, of several hundred to a few thousand solar masses with a typical size of 0.1–1 pc), such as dust temperature ...
    • SiO outflows in high-mass star forming regions: A potential chemical clock? 
      López Sepulcre, A.; Walmsley, C. M.; Cesaroni, R.; Codella, C.; Schuller, F.; Bronfman Aguiló, Leonardo; Carey, S. J.; Menten, K. M.; Molinari, S.; Noriega Crespo, A. (EDP SCIENCES, 2011-02)
      Context. Some theoretical models propose that O-B stars form via accretion, in a similar fashion to low-mass stars. Jet-driven molecular outflows play an important role in this scenario, and their study can help to understand ...