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The impact of the SKA on Galactic Radioastronomy: continuum observations
Grazia Umana, Corrado Trigilio, Luciano Cerrigone +11
The SKA will be a state of the art radiotelescope optimized for both large area surveys as well as for deep pointed observations. In this paper we analyze the impact that the SKA w…
The YSO Population in the Vela-D Molecular Cloud
F. Strafella, D. Lorenzetti, T. Giannini +7
We investigate the young stellar population in the Vela Molecular Ridge, Cloud-D (VMR-D), a star forming (SF) region observed by both Spitzer/NASA and Herschel/ESA space telescope.…
A necklace of dense cores in the high-mass star forming region G35.20-0.74N: ALMA observations
Á. Sánchez-Monge, M. T. Beltrán, R. Cesaroni +13
The present study aims at characterizing the massive star forming region G35.20N, which is found associated with at least one massive outflow and contains multiple dense cores, one…
GAMMA-LIGHT: High-Energy Astrophysics above 10 MeV
Aldo Morselli, Andrea Argan, Guido Barbiellini +39
High-energy phenomena in the cosmos, and in particular processes leading to the emission of gamma- rays in the energy range 10 MeV - 100 GeV, play a very special role in the unders…
The molecular complex associated with the Galactic HII region Sh2-90: a possible site of triggered star formation
M. R. Samal, A. Zavagno, L. Deharveng +6
We investigate the star formation activity in the molecular complex associated with the Galactic HII region Sh2-90, using radio-continuum maps obtained at 1280 MHz and 610 MHz, Her…
The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30,0)
Alessio Traficante, Roberta Paladini, Mathieu Compiegne +13
Herschel FIR continuum data obtained as part of the Hi-GAL survey have been used, together with the GLIMPSE 8 m and MIPSGAL 24 m data, to attempt the first 3D-decomposition o…