activity
20002005
most citedGLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy

1.4k citations · 1.7k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2005★ 28 cited

Identification of Main Sequence Stars with Mid-Infrared Excesses Using GLIMPSE: Beta-Pictoris Analogs?

B. Uzpen, H. A. Kobulnicky, K. A. G. Olsen +23

Spitzer IRAC 3.6-8 micron photometry obtained as part of the GLIMPSE survey has revealed mid-infrared excesses for 33 field stars with known spectral types in a 1.2 sq. degree fiel…

astro-ph2004★ 77 cited

A GLIMPSE of Star Formation in the Giant H II Region RCW 49

B. A. Whitney, R. Indebetouw, B. L. Babler +19

GLIMPSE imaging using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope indicates that star formation is ongoing in the RCW 49 giant H II region. A photometric compar…

astro-ph2004★ 23 cited

Dust heating by the interstellar radiation field in models of turbulent molecular clouds

Thomas Bethell, Ellen Zweibel, Fabian Heitsch +1

We have calculated the radiation field, dust grain temperatures, and far infrared emissivity of numerical models of turbulent molecular clouds. When compared to a uniform cloud of…

astro-ph2003★ 1.4k cited

GLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy

Robert A. Benjamin, E. Churchwell, Brian L. Babler +17

GLIMPSE (Galactic Legacy Infrared Mid-Plane Survey Extraordinaire), a SIRTF Legacy Science Program, will be a fully sampled, confusion-limited infrared survey of the inner two-thir…

astro-ph2001★ 133 cited

ISO spectroscopy of compact HII regions in the Galaxy. II Ionization and elemental abundances

N. L. Martin-Hernandez, E. Peeters, C. Morisset +9

Based on the ISO spectral catalogue of compact HII regions by Peeters et al. (2001), we present a first analysis of the hydrogen recombination and atomic fine-structure lines origi…

astro-ph2000★ 78 cited

Dependence of Gas Phase Abundances in the ISM on Column Density

B. P. Wakker, J. S. Mathis

Sightlines through high- and intermediate-velocity clouds allow measurements of ionic gas phase abundances, A, at very low values of HI column density, N(HI). Present observations…