activity
20202025
most citedPhysical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations

48 citations · 92 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.IM2025

Sub-millimeter wavelength protostellar accretion rate monitoring with AtLAST

Thomas Stanke, Verena Wolf, Bringfried Stecklum +5

How a star forms is a fundamental question in astrophysics. In the earliest stages of protostellar evolution high extinction prevents a direct study of the accretion processes and…

astro-ph.IM2024

A low-cost, high-speed, very high-order Shack-Hartmann sensor for testing TMT deformable mirrors

Mojtaba Taheri, David Andersen, Jean-Pierre Veran +1

The Thirty Meter Telescope will use a sophisticated adaptive optics system called NFIRAOS. This system utilizes two deformable mirrors conjugate to 0 km and 11.2 km to apply a Mult…

astro-ph.GA2022★ 26 cited

Evidence of ram pressure stripping of WLM, a dwarf galaxy far away from any large host galaxy

Yanbin Yang, Roger Ianjamasimanana, Francois Hammer +5

Dwarf galaxies are affected by all the evolutionary processes normally at work in galaxies of any mass. As fainter and less massive galaxies, however, dwarf galaxies are particular…

astro-ph.GA2020★ 18 cited

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). VIII. Modeling ram pressure stripping of diffuse gas in the Virgo cluster spiral galaxy NGC 4330

B. Vollmer, M. Fossati, A. Boselli +7

NGC 4330 is one of the Virgo galaxies whose UV distribution shows a tail structure. An associated tail structure is also observed in the HI and H emission distributions. Previou…

astro-ph.GA2020★ 48 cited

Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations

S. Pezzuto, M. Benedettini, J. Di Francesco +20

(Abridged) In this paper, we present analyses of images taken with the Herschel ESA satellite from 70mu to 500mu. We first constructed column density and dust temperature maps. Nex…