most citedSimultaneous Determination of the Cosmic Ray Ionization Rate and Fractional Ionization in DR21(OH)

44 citations · 103 across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph200828 cited

Dichotomy in the Dynamical Status of Massive Cores in Orion

T. velusamy, R. Peng, D. Li +2

To study the evolution of high mass cores, we have searched for evidence of collapse motions in a large sample of starless cores in the Orion molecular cloud. We used the Caltech S…

astro-ph200844 cited

Simultaneous Determination of the Cosmic Ray Ionization Rate and Fractional Ionization in DR21(OH)

T. Hezareh, M. Houde, C. McCoey +2

We present a new method for the simultaneous calculation of the cosmic ray ionization rate, zeta(H2), and the ionization fraction, chi(e), in dense molecular clouds. A simple netwo…

astro-ph200831 cited

An Upper Limit on Gas Production from 3200 Phaethon

Paul A. Wiegert, Martin Houde, Ruisheng Peng

Asteroid 3200 Phaethon resembles a comet in some ways, including a highly-eccentric orbit (e=0.89) and a strong associated meteor shower (the Geminids). Yet this object has never b…

astro-ph2003

Tracing the Magnetic Field in Orion A

Martin Houde, C. Darren Dowell, Roger. H. Hildebrand +5

We use extensive 350 um polarimetry and continuum maps obtained with Hertz and SHARC II along with HCN and HCO+ spectroscopic data to trace the orientation of the magnetic field in…

astro-ph2003

On the Measurement of the Magnitude and Orientation of the Magnetic Field in Molecular Clouds

Martin Houde, Pierre Bastien, Jessie L. Dotson +6

We demonstrate that the combination of Zeeman, polarimetry and ion-to-neutral molecular line width ratio measurements permits the determination of the magnitude and orientation of…

astro-ph2003

The Alignment of the Magnetic Field and Collimated Outflows in Star-forming Regions: the Case of NGC 2071

Martin Houde, Thomas G. Phillips, Pierre Bastien +2

The magnetic field is believed to play a crucial role in the process of star formation. From the support it provides during the initial collapse of molecular clouds to the creation…