E. Sciacca

activity

20102017

most citedProperties 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}

)

201 citations · 400 across the 4 of their papers we have counts for

collaborators

Showing astro-ph.GAShow all

3 papers · 1 filter

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★ 36 cited

Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane

P. Palmeirim, A. Zavagno, D. Elia +35

We present a comprehensive statistical analysis of star-forming objects located in the vicinities of 1 360 bubble structures throughout the Galactic Plane and their local environme…

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∘)

Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane

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