201 citations · 287 across the 7 of their papers we have counts for
7 papers
Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()
D. Elia, S. Molinari, E. Schisano +83
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 m. We present a band-merged catalogue of spatia…
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.…
XMM-Newton and Swift observations of WZ Sge: spectral and timing analysis
A. A. Nucita, E. Kuulkers, F. De Paolis +3
WZ Sagittae is the prototype object of a subclass of dwarf novae, with rare and long (super)outbursts, in which a white dwarf primary accretes matter from a low mass companion. Hig…
Spitzer-IRAC survey of molecular jets in Vela-D
T. Giannini, D. Lorenzetti, M. De Luca +10
We present a survey of H2 jets from young protostars in the Vela-D molecular cloud (VMR-D), based on Spitzer -IRAC data between 3.6 and 8.0 micron. Our search has led to the identi…
The X-ray eclipse of the dwarf nova HT CAS observed by the XMM-Newton satellite: spectral and timing analysis
A. A. Nucita, B. M. T. Maiolo, S. Carpano +5
A cataclysmic variable is a binary system consisting of a white dwarf that accretes material from a secondary object via the Roche-lobe mechanism. In the case of long enough observ…
XMM-Newton observation of MACHO 104.20906.960: a dwarf nova candidate with a 2 h period
A. A. Nucita, S. Carpano, F. De Paolis +3
The binaries known as cataclysmic variables are particular binary systems in which the primary star (a white dwarf) accretes material from a secondary via Roche-lobe mechanism. Usu…
Mapping molecular emission in Vela Molecular Ridge Cloud D
D. Elia, F. Massi, F. Strafella +6
We present the 12CO(1-0) and 13CO(2-1) line maps obtained observing with the SEST a $\sim 1\degr \times 1\degr$ region of the Vela Molecular Ridge, Cloud D. This cloud is part of a…