output
19972026
most citedThe Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

7.7k citations

Showing 2018 · astro-ph.GAShow all

23 papers · 2 filters

astro-ph.GA2018★ 14 cited

Characterising the high-mass star forming filament G351.776--0.527 with Herschel and APEX dust continuum and gas observations

S. Leurini, E. Schisano, T. Pillai +13

G351.776-0.527 is among the most massive, closest, and youngest filaments in the inner Galactic plane and therefore it is an ideal laboratory to study the kinematics of dense gas a…

astro-ph.GA2018★ 37 cited

The Formation Conditions of the Wide Binary Class 0 Protostars within BHR 71

John Tobin, Tyler Bourke, Stacy Mader +7

We present a characterization of the binary protostar system that is forming within a dense core in the isolated dark cloud BHR71. The pair of protostars, IRS1 and IRS2, are both i…

astro-ph.GA2018★ 96 cited

The ALMA Fornax Cluster Survey I: stirring and stripping of the molecular gas in cluster galaxies

Nikki Zabel, Timothy A. Davis, Matthew W. L. Smith +15

We present the first results of the ALMA Fornax Cluster Survey (AlFoCS): a complete ALMA survey of all members of the Fornax galaxy cluster that were detected in HI or in the far i…

astro-ph.GA2018★ 31 cited

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).V. Properties of the ionised gas filament of M87

A. Boselli, M. Fossati, A. Longobardi +22

We have observed the giant elliptical galaxy M87 during the Virgo Environmental Survey Tracing Galaxy Evolution (VESTIGE), a blind narrow-band Halpha+[NII] imaging survey of the Vi…

astro-ph.GA2018★ 35 cited

LOFAR MSSS: Flattening low-frequency radio continuum spectra of nearby galaxies

K. T. Chyży, W. Jurusik, J. Piotrowska +35

The shape of low-frequency radio continuum spectra of normal galaxies is not well understood, the key question being the role of physical processes such as thermal absorption in sh…

astro-ph.GA2018★ 46 cited

SEDIGISM: The kinematics of ATLASGAL filaments

M. Mattern, J. Kauffmann, T. Csengeri +13

Analysing the kinematics of filamentary molecular clouds is a crucial step towards understanding their role in the star formation process. Therefore, we study the kinematics of 283…