activity
20102026
most citedDistance Determinations to SHIELD Galaxies from HST Imaging

37 citations · 91 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

The Neutral Atomic Hydrogen in the solar neighborhood (NeAtHood) project I. Ghost in the shell: Neutral atomic hydrogen in the extended Orion nebula

J. D. Soler, H. Beuther, S. C. O. Glover +15

The Orion Nebula is the nearest site of ongoing and recent high-mass star formation. It is a unique laboratory for studying the mass, energy, and momentum input from high-mass star…

astro-ph.GA2023★ 16 cited

A global view on star formation: The GLOSTAR Galactic plane survey. IX. Radio Source Catalog III: 2<l<28, 36<l<40, 56<l<60 and |b|<1, VLA B-configuration

A. Y. Yang, S. A. Dzib, J. S. Urquhart +20

As part of the GLOSTAR (GLObal view of STAR formation in the Milky Way) survey, we present the high-resolution continuum source catalog for the regions (l = 2-28, 36-40, 56-60, &|b…

astro-ph.GA2022

A global view on star formation: The GLOSTAR Galactic plane survey. VII. Supernova remnants in the Galactic longitude range

R. Dokara, Y. Gong, W. Reich +19

Context. While over 1000 supernova remnants (SNRs) are estimated to exist in the Milky Way, only less than 400 have been found to date. In the context of this apparent deficiency,…

astro-ph.GA2022

A global view on star formation: The GLOSTAR Galactic plane survey. VI. Radio Source Catalog II: and , VLA B-configuration

S. A. Dzib, A. Y. Yang, J. S. Urquhart +20

As part of the GLOSTAR survey we have used the VLA in its B-configuration to observe the part of the Galactic plane between longitudes of 28d and 36d and latitudes from -1d to +1d…

astro-ph.GA2022★ 7 cited

Evidence for an interaction between the Galactic Center clouds M0.10-0.08 and M0.11-0.11

Natalie O. Butterfield, Cornelia C. Lang, Adam Ginsburg +3

We present high-resolution (~2-3"; ~0.1 pc) radio observations of the Galactic center cloud M0.10-0.08 using the Very Large Array at K and Ka band (~25 and 36 GHz). The M0.10-0.08…

astro-ph.GA2021★ 22 cited

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde IV. The ALMA view of N113 and N159W in the LMC

X. D. Tang, C. Henkel, K. M. Menten +25

We mapped the kinetic temperature structure of two massive star-forming regions, N113 and N159W, in the Large Magellanic Cloud (LMC). We have used 1\hbox{$\,.\!\!^{\prime\pri…

astro-ph.GA2014★ 37 cited

Distance Determinations to SHIELD Galaxies from HST Imaging

Kristen. B. W. McQuinn, John M. Cannon, Andrew E. Dolphin +9

The Survey of HI in Extremely Low-mass Dwarf galaxies (SHIELD) is an on-going multi-wavelength program to characterize the gas, star formation, and evolution in gas-rich, very low-…

astro-ph.SR2010★ 9 cited

A study of three southern high-mass star-forming regions

C. Dedes, S. Leurini, F. Wyrowski +4

Based on color-selected IRAS point sources, we have started to conduct a survey of 47 high-mass star-forming regions in the southern hemisphere in 870um dust continuum and molecula…