activity
19972004
most citedFeedback and Formation of Massive Star Clusters in Giant Molecular Clouds

1 citations · 1 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph2004

A New Kind of Nova

J. L. Sokoloski, S. J. Kenyon, A. K. H. Kong +10

We performed extensive, multi-wavelength observations of the prototypical symbiotic star Z Andromedae between 2000 and 2003, during a large eruption. The rise to optical maximum oc…

astro-ph20041 cited

Feedback and Formation of Massive Star Clusters in Giant Molecular Clouds

Jonathan C. Tan, Christopher F. McKee

It is well known that the energy input from massive stars dominates the thermal and mechanical heating of typical regions in the interstellar medium of galaxies. These effects are…

astro-ph2003

Outflow-Confined HII Regions and the Formation of Massive Stars by Accretion

Jonathan C. Tan, Christopher F. McKee

If massive stars form by disk accretion, then bipolar outflows should be generated as in the case of low-mass star formation. High accretion rates lead to high outflow rates and ma…

astro-ph2002

The Formation of Massive Stars and Star Clusters

Jonathan C. Tan, Christopher F. McKee

We model the formation of high-mass stars, specifying the accretion rate in terms of the instantaneous and final mass of the star, the ambient pressure of the star-forming region a…

astro-ph2000

The Genesis of Super Star Clusters as Self-Gravitating HII Regions

Jonathan C. Tan, Christopher F. McKee

We examine the effects of ionization, radiation pressure and main sequence winds from massive stars on self-gravitating, clumpy molecular clouds, thereby modeling the formation and…

astro-ph2000

An accelerated Monte Carlo method to solve two-dimensional radiative transfer and molecular excitation

Michiel R. Hogerheijde, Floris F. S. van der Tak

We present a numerical method and computer code to calculate the radiative transfer and excitation of molecular lines. Formulating the Monte Carlo method from the viewpoint of cell…