L. Cambr'esy

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 · 320 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2019★ 83 cited

The Hi-GAL catalogue of dusty filamentary structures in the Galactic Plane

E. Schisano, S. Molinari, D. Elia +27

The recent data collected by {\it Herschel} have confirmed that interstellar structures with filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to b…

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…

The Hi-GAL catalogue of dusty filamentary structures in the 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∘<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 ( $- 71. 0^{\circ} < ℓ < 67. 0^{\circ}$ )