Browsing by Author "Pezzuto, S."

Now showing items 1-4 of 4

    • Distance of Hi-GAL sources 
      Mège, P.; Russeil, D.; Zavagno, A.; Elia, D.; Molinari, S.; Brunt, C. M.; Butora, R.; Cambresy, L.; Di Giorgio, A. M.; Fenouillet, T.; Fukui, Y.; Lambert, J. C.; Makai, Z.; Merello, Manuel; Meunier, J.C.; Molinaro, M.; Moreau, C.; Pezzuto, S.; Poulin, Y.; Schisano, E.; Schuller, F. (EDP Sciences S A, 2021)
      Aims. Distances are key to determining the physical properties of sources. In the Galaxy, large (>10 000) homogeneous samples of sources for which distance are available, covering the whole Galactic distance range, are ...
    • Ionisation impact of high-mass stars on interstellar filaments A Herschel study of the RCW36 bipolar nebula ... 
      Minier, V.; Tremblin, P.; Hill, T.; Motte, F.; André, Ph.; Lo, N.; Schneider, N.; Audit, E.; White, G. J.; Hennemann, M.; Cunningham, M.; Deharveng, L.; Di Francesco, J.; Elia, D.; Giannini, T.; Luong, Q. Nguyen; Pezzuto, S.; Rygl, K. L.; Spinoglio, L.; Ward Thompson, D.; Zavagno, A. (EDP Sciences, 2013)
      Context. Ionising stars reshape their original molecular cloud and impact star formation, leading to spectacular morphologies such as bipolar nebulae around Hii regions. Molecular clouds are structured in filaments where ...
    • 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 ...
    • Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core ... 
      Roy, A.; André, Ph.; Arzoumanian, D.; Peretto, N.; Palmeirim, P.; Könyves, V.; Schneider, N.; Benedettini, M.; Di Francesco, J.; Elia, D.; Hill, T.; Ladjelate, B.; Louvet, F.; Motte, F.; Pezzuto, S.; Schisano, E.; Shimajiri, Y.; Spinoglio, L.; Ward Thompson, D.; White, G. (EDP Sciences, 2015)
      A complete understanding of the origin of the prestellar core mass function (CMF) is crucial. Two major features of the prestellar CMF are 1) a broad peak below 1M(circle dot), presumably corresponding to a mean gravitational ...