D. Elia

activity

20062026

most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 6.7k across the 92 of their papers we have counts for

collaborators

Showing 2017 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2017★ 157 cited

Multi-temperature mapping of dust structures throughout the Galactic Plane using the PPMAP tool with Herschel Hi-GAL data

K. A. Marsh, A. P. Whitworth, O. Lomax +13

We describe new Hi-GAL based maps of the entire Galactic Plane, obtained using continuum data in the wavelength range 70-500 $μ$ m. These maps are derived with the PPMAP procedure,…

astro-ph.GA2017★ 201 cited

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 ( $- 71. 0^{\circ} < ℓ < 67. 0^{\circ}$ )

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 $μ$ m. We present a band-merged catalogue of spatia…

astro-ph.GA2017★ 38 cited

Distance biases in the estimation of the physical properties of Hi-GAL compact sources-I. Clump properties and the identification of high-mass star forming candidates

Adriano Baldeschi, Davide Elia, Sergio Molinari +8

The degradation of spatial resolution in star-forming regions observed at large distances ( $d ≳ 1$ kpc) with Herschel,can lead to estimates of the physical parameters of the de…

Multi-temperature mapping of dust structures throughout the Galactic Plane using the PPMAP tool with Herschel Hi-GAL data

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 (−71.0∘<ℓ<67.0∘)

Distance biases in the estimation of the physical properties of Hi-GAL compact sources-I. Clump properties and the identification of high-mass star forming candidates

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 ( $- 71. 0^{\circ} < ℓ < 67. 0^{\circ}$ )