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20032008
most citedHigh Resolution =1mm CARMA Observations of Large Molecules in Orion-KL

40 citations · 94 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph200821 cited

The Distribution, Excitation and Formation of Cometary Molecules: Methanol, Methyl Cyanide and Ethylene Glycol

Anthony J. Remijan, Stefanie N. Milam, Maria Womack +12

We present an interferometric and single dish study of small organic species toward Comets C/1995 O1 (Hale-Bopp) and C/2002 T7 (LINEAR) using the BIMA interferometer at 3 mm and th…

astro-ph200740 cited

High Resolution =1mm CARMA Observations of Large Molecules in Orion-KL

D. N. Friedel, L. E. Snyder

We present high resolution, Combined Array for Research in Millimeter-Wave Astronomy (CARMA), =1mm observations of several molecular species toward Orion-KL. These are the highe…

astro-ph200633 cited

A Bima Array Survey of Molecules in Comets Linear (C/2002 T7) and Neat (C/2001 Q4)

Anthony J. Remijan, D. N. Friedel, Imke de Pater +10

We present an interferometric search for large molecules, including methanol, methyl cyanide, ethyl cyanide, ethanol, and methyl formate in comets LINEAR (C/2002 T7) and NEAT (C/20…

astro-ph2005

Detection of Interstellar Acetone Toward the Orion-KL Hot Core

D. N. Friedel, L. E. Snyder, Anthony J. Remijan +1

We present the first detection of interstellar acetone [(CH3)2CO] toward the high mass star forming region Orion-KL and the first detection of vibrationally excited (CH3)2CO in the…

astro-ph2005

BIMA Array Detections of HCN in Comets LINEAR (C/2002 T7) and NEAT (C/2001 Q4)

D. N. Friedel, Anthony J. Remijan, L. E. Snyder +10

We present interferometric detections of HCN in comets LINEAR (C/2002 T7) and NEAT (C/2001 Q4) with the Berkeley-Illinois-Maryland Association (BIMA) Array. With a 25.4"x20.3" synt…

astro-ph2004

A Rigorous Attempt to Verify Interstellar Glycine

L. E. Snyder, F. J. Lovas, J. M. Hollis +6

In 2003, Kuan, Charnley, and co-workers reported the detection of interstellar glycine (NH2CH2COOH) based on observations of 27 lines in 19 different spectral bands in one or more…