activity
19992023
most citedHerschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?

595 citations · 3.3k across the 60 of their papers we have counts for

collaborators

61 papers

astro-ph.GA2023★ 5 cited

Mapping the multiphase structure of H I in the Low-Latitude Intermediate-Velocity Arch 1

Luka Vujeva, Antoine Marchal, Peter G. Martin +1

We have analyzed the thermal and turbulent properties of the Low-Latitude Intermediate-Velocity Arch 1 (LLIV1). This was accomplished using archival H I emission and absorption dat…

astro-ph.GA2023★ 14 cited

Joint Modelling of Dust Scattering and Thermal Emission: The Spider Complex

Jielai Zhang, Peter G Martin, Ryan Cloutier +4

Observations across the electromagnetic spectrum of radiative processes involving interstellar dust -- emission, extinction, and scattering -- are used to constrain the parameters…

astro-ph.GA2022★ 11 cited

Mapping the Thermal Condensation of Diffuse H I in the North Celestial Pole Loop

Mukesh Taank, Antoine Marchal, Peter G. Martin +1

The North Celestial Pole Loop (NCPL) provides a unique laboratory for studying the early stages of star formation, in particular the condensation of the neutral interstellar medium…

astro-ph.IM2021★ 20 cited

A Method To Characterize the Wide-Angle Point Spread Function of Astronomical Images

Qing Liu, Roberto Abraham, Colleen Gilhuly +14

Uncertainty in the wide-angle Point Spread Function (PSF) at large angles (tens of arcseconds and beyond) is one of the dominant sources of error in a number of important quantitie…

astro-ph.GA2021★ 25 cited

Are massive dense clumps truly sub-virial? A new analysis using Gould Belt ammonia data

Ayushi Singh, Christopher D. Matzner, Rachel K. Friesen +21

Dynamical studies of dense structures within molecular clouds often conclude that the most massive clumps contain too little kinetic energy for virial equilibrium, unless they are…

astro-ph.GA2021★ 1 cited

Resolving the formation of cold HI filaments in the high velocity cloud complex C

Antoine Marchal, Peter G. Martin, Munan Gong

The physical properties of galactic halo gas have a profound impact on the life cycle of galaxies. As gas travels through a galactic halo, it undergoes dynamical interactions, infl…