activity
19962021
most citedSINGS: The SIRTF Nearby Galaxies Survey

1.3k citations · 15.4k across the 98 of their papers we have counts for

collaborators

99 papers

astro-ph.GA2021★ 31 cited

CO emission as an effective measure of gas masses of protoplanetary disks

Maxime Ruaud, Uma Gorti, David Hollenbach

Many astrochemical models of observed CO isotopologue line emission, earlier considered a good proxy measure of H and hence disk gas mass, favor large deviations in the carbon…

astro-ph.GA2020★ 8 cited

Distribution of Water Vapor in Molecular Clouds. II

Gary J. Melnick, Volker Tolls, Ronald L. Snell +8

The depth-dependent abundance of both gas-phase and solid-state water within dense, quiescent, molecular clouds is important to both the cloud chemistry and gas cooling. Where wate…

astro-ph.GA2019★ 21 cited

Probing ISM Structure in Trumpler 14 & Carina I Using The Stratospheric Terahertz Observatory 2

Young Min Seo, Paul F. Goldsmith, Chris Walker +26

We present observations of the Trumpler 14/Carina I region carried out using the Stratospheric Terahertz Observatory 2 (STO2). The Trumpler 14/Carina I region is in the west part o…

astro-ph.GA2018★ 8 cited

The High Mass Slope of the IMF

Antonio Parravano, David Hollenbach, Christopher F. McKee

Recent papers have found that the inferred slope of the high-mass ( M) IMF for field stars in the solar vicinity has a larger value () than the slopes (…

astro-ph.EP2017★ 3 cited

A likely planet-induced gap in the disk around T Cha

Nathanial P. Hendler, Paola Pinilla, Ilaria Pascucci +7

We present high resolution () 3mm ALMA observations of the highly inclined transition disk around the star T Cha. Our continuum image reveals multiple dust struct…

astro-ph.SR2016★ 135 cited

Tracing Slow Winds from T Tauri Stars via Low Velocity Forbidden Line Emission

M. N. Simon, I. Pascucci, S. Edwards +5

Using Keck/HIRES spectra Δv ~ 7 km/s, we analyze forbidden lines of [O I] 6300 Å, [O I] 5577 Å and [S II] 6731 Å from 33 T Tauri stars covering a range of disk evolutionary stages.…