Browsing by Author "Olmi, L."

Now showing items 1-3 of 3

    • An H2Co 6 cm maser pinpointing a possible circumstellar torus in IRAS 18566+0408 
      Araya, E.; Hofner, P.; Sewixo, M.; Goss, W. M.; Linz, H.; Kurtz, S.; Olmi, L.; Churchwell, E.; Rodríguez, L. F.; Garay Brignardello, Guido (UNIV CHICAGO PRESS, 2007-11-10)
      We report observations of 6 cm, 3.6 cm, 1.3 cm, and 7 mm radio continuum, conducted with the Very Large Array, toward IRAS 18566+0408, one of the few sources known to harbor H(2)CO6 cm maser emission. Our observations ...
    • Molecular cloud catalogue from (CO)-C-13 (1-0) data of the Forgotten Quadrant Survey 
      Benedettini, M.; Traficante, A.; Olmi, L.; Pezzuto, S.; Baldeschi, A.; Molinari, S.; Elia, D.; Schisano, E.; Merello, M.; Fontani, F.; Rygl, K. L. J.; Brand, J.; Beltrán, M. T.; Cesaroni, R.; Liu, S. J.; Testi, L. (EDP Sciences, 2021)
      Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structure of the interstellar medium, allowing the simultaneous study of dense structures from single star-forming objects or ...
    • The molecular environment of the Galactic star forming region G19.61–0.23 
      Santangelo, G.; Testi, L.; Leurini, S.; Walmsley, C. M.; Cesaroni, R.; Bronfman Aguiló, Leonardo; Carey, S.; Gregorini, L.; Menten, K. M.; Molinari, S.; Noriega Crespo, A.; Olmi, L.; Schuller, F. (ESO, 2010-06-03)
      Context. Although current facilities allow the study of Galactic star formation at high angular resolution, our current understanding of the high-mass star-formation process is still very poor. In particular, we still ...