activity
19962007
most citedA Comparison of the Morphology and Stability of Relativistic and Nonrelativistic Jets

73 citations · 478 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph2007★ 17 cited

Interacting Jets from Binary Protostars

G. C. Murphy, T. Lery, S. O'Sullivan +3

We investigate potential models that could explain why multiple proto-stellar systems predominantly show single jets. During their formation, stars most frequently produce energeti…

astro-ph2006★ 50 cited

Outflows from the high-mass protostars NGC 7538 IRS1/2 observed with bispectrum speckle interferometry -- Signatures of flow precession

S. Kraus, Y. Balega, M. Elitzur +6

NGC 7538 IRS1 is a high-mass (approx. 30 M_sun) protostar with a CO outflow, an associated UCHII region, and a linear methanol maser structure, which might trace a Keplerian-rotati…

astro-ph2006★ 26 cited

Molecular Outflows in Low- and High-Mass Star Forming Regions

Hector G. Arce, Debra Shepherd, Frederic Gueth +4

We review the known properties of molecular outflows from low- and high-mass young stars. General trends among outflows are identified, and the most recent studies on the morpholog…

astro-ph2004★ 27 cited

Hydrodynamic simulations of molecular outflows driven by slow-precessing protostellar jets

Michael D. Smith, Alex Rosen

We present hydrodynamic simulations of molecular outflows driven by jets with a long period of precession, motivated by observations of arc-like features and S-symmetry in outflows…

astro-ph2003★ 18 cited

Simulations of Evolving or Outbursting Molecular Protostellar Jets

Alexander Rosen, Michael D. Smith

The kinematic and radiative power of molecular jets is expected to change as a protostar undergoes permanent or episodal changes in the rate at which it accretes. We study here the…

astro-ph2002★ 37 cited

Hydrodynamical simulations of the decay of high-speed molecular turbulence. I. Dense molecular regions

Georgi Pavlovski, Michael D. Smith, Mordecai-Mark Mac Low +1

We present the results from three dimensional hydrodynamical simulations of decaying high-speed turbulence in dense molecular clouds. We compare our results, which include a detail…