Showing 1–15 of 15 results
/ Date/ Name
Dec 15, 2016An analysis of star formation with Herschel in the Hi-GAL Survey. II. The tips of the Galactic barNov 11, 2014The YSO Population in the Vela-D Molecular CloudApr 8, 2014Characterizing the structure of diffuse emission in Hi-GAL mapsMar 7, 2025ALMAGAL III. Compact source catalog: Fragmentation statistics and physical evolution of the core populationFeb 14, 2013Spitzer-IRAC survey of molecular jets in Vela-DNov 13, 2025ALMAGAL V. Relations between the core populations and the parent clump physical propertiesApr 27, 2013The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5Oct 7, 2009Analysis of the fraction of clear sky at the La Palma and Mt Graham sitesNov 10, 2022The Star Formation Rate of the Milky Way as seen by HerschelMar 5, 2010A characterization of the NGC 4051 soft X-ray spectrum as observed by XMM-NewtonAug 15, 2024Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clustersDec 5, 2025ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clumpNov 22, 2010Fraction of clear skies above astronomical sites: a new analysis from the GOES12 satelliteApr 29, 2022Latent Space Explorer: Unsupervised Data Pattern Discovery on the CloudJun 4, 2017Properties 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 ($-71.0^{\circ}< \ell < 67.0^{\circ}$)