activity
20092026
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 6.4k across the 118 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.IM2023★ 4 cited

A new tool to derive simultaneously exponent and extremes of power-law distributions

S. Pezzuto, A. Coletta, R. S. Klessen +6

Many experimental quantities show a power-law distribution . In astrophysics, examples are: size distribution of dust grains or luminosity function of galaxies.…

astro-ph.GA2023★ 13 cited

A comparison of the Milky Way's recent star formation revealed by dust thermal emission and high-mass stars

J. D. Soler, E. Zari, D. Elia +10

We present a comparison of the Milky Way's star formation rate (SFR) surface density () obtained with two independent state-of-the-art observational methods. The first…

astro-ph.GA2023

Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS)

Roberta Paladini, Catherine Zucker, Robert Benjamin +67

A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is supported by a large representation of the community of Galactic astronomers. The combination of sensitiv…

astro-ph.GA2023★ 14 cited

A panoptic view of the Taurus molecular cloud I. The cloud dynamics revealed by gas emission and 3D dust

J. D. Soler, C. Zucker, J. E. G. Peek +14

We present a study of the three-dimensional (3D) distribution of interstellar dust derived from stellar extinction observations toward the Taurus molecular cloud (MC) and its relat…

astro-ph.GA2023★ 35 cited

The SQUALO project (Star formation in QUiescent And Luminous Objects) I: clump-fed accretion mechanism in high-mass star-forming objects

A. Traficante, B. M. Jones, A. Avison +10

The formation mechanism of the most massive stars is far from completely understood. It is still unclear if the formation is core-fed or clump-fed, i.e. if the process is an extens…

astro-ph.EP2023★ 24 cited

Oxygen depletion in giant planets with different formation histories

S. Fonte, D. Turrini, E. Pacetti +5

The atmospheric C/O ratio of exoplanets is widely used to constrain their formation. To guarantee that the C/O ratio provides robust information, we need to accurately quantify the…