22k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Massachusetts Institute of TechnologyUS255 papers
- California Institute of TechnologyUS233 papers
- Triangle Universities Nuclear LaboratoryUS232 papers
- Center for Astrophysics Harvard & SmithsonianUS218 papers
- Duke UniversityUS195 papers
- University of California, BerkeleyUS186 papers
- Lawrence Berkeley National LaboratoryUS185 papers
- Centre National de la Recherche ScientifiqueFR182 papers
- University of WashingtonUS182 papers
- Princeton UniversityUS178 papers
- The University of Texas at AustinUS168 papers
- Vanderbilt UniversityUS159 papers
6 papers · 2 filters
Galaxies M32 and NGC 5102 Confirm a Near-infrared Spectroscopic Chronometer
Jesse Miner, James A. Rose, Gerald Cecil
We present near infrared (NIR) IRTF/SpeX spectra of the intermediate-age galaxy M32 and the post-starburst galaxy NGC 5102. We show that features from thermally-pulsing asymptotic…
Formation of Cold Filamentary Structure from Wind Blown Superbubbles
Evangelia Ntormousi, Andreas Burkert, Katharina Fierlinger +1
The expansion and collision of two wind-blown superbubbles is investigated numerically. Our models go beyond previous simulations of molecular cloud formation from converging gas f…
Physical Properties of Complex C Halo Clouds
W. -H. Hsu, M. E. Putman, F. Heitsch +3
Observations from the Galactic Arecibo L-Band Feed Array HI (GALFA-HI) Survey of the tail of Complex C are presented and the halo clouds associated with this complex cataloged. The…
Gravity or Turbulence? The velocity dispersion-size relation
Javier Ballesteros-Paredes, Lee W. Hartmann, Enrique Vázquez-Semadeni +2
We discuss the nature of the velocity dispersion vs. size relation for molecular clouds. In particular, we add to previous observational results showing that the velocity dispersio…
Morphological Complexity of Protostellar Envelopes
John J. Tobin, Lee Hartmann, Edwin Bergin +3
Extinction maps at 8 micron from the Spitzer Space Telescope show that many Class 0 protostars exhibit complex, irregular, and on-axisymmetric structure within the densest regions…
Spitzer View of Young Massive Stars in the LMC HII Complexes. II. N159
C. -H. Rosie Chen, Remy Indebetouw, You-Hua Chu +6
The HII complex N159 in the Large Magellanic Cloud (LMC) is used to study massive star formation in different environments, as it contains three giant molecular clouds (GMCs) that…