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Thomas G. Phillips

Researcher at California Institute of Technology

Publications -  477
Citations -  21382

Thomas G. Phillips is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Caltech Submillimeter Observatory & Molecular cloud. The author has an hindex of 77, co-authored 477 publications receiving 20630 citations. Previous affiliations of Thomas G. Phillips include Bayer & ASTRON.

Papers
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G34.24+0.13MM: A Deeply Embedded Proto-B-Star

Todd R. Hunter, +6 more
- 01 Feb 1998 - 
TL;DR: By means of millimeter and submillimeter imaging, a massive protostellar object that coincides with a methanol maser and is not detectable in the continuum at centimeter wavelengths was identified in this article.
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Radio-Frequency Continuum Emission from Evolved Stars

Gillian R. Knapp, +3 more
- 01 Dec 1995 - 
TL;DR: In this article, the evolution of stars between the AGB and planetary nebula phases was investigated by sensitive radio continuum observations of a sample of 21 evolved stars with high mass loss rates and extended circumstellar envelopes, in a search for newly formed compact planetary nebulae.
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Filamentary Structure and Helical Magnetic Fields in the Environment of a Starless Dense Core

Edith Falgarone, +2 more
- 01 Jul 2001 - 
TL;DR: In this article, the authors have shown that the toroidal component of the magnetic field dominates the poloidal component, which may be a signature of magnetohydrodynamic instability developing in filaments permeated by a helical magnetic field.
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Atomic Carbon in the Envelope of IRC +10216

Jocelyn Keene, +4 more
- 01 Oct 1993 - 
TL;DR: In this article, the 3 P 1 → 3 P 0 transition of atomic carbon at 492 GHz in IRC+10216 was observed at the Caltech Submillimeter Observatory.
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First detections of the [NII] 122 {\mu}m line at high redshift: Demonstrating the utility of the line for studying galaxies in the early universe

Carl Ferkinhoff, +9 more
- 07 Sep 2011 - 
TL;DR: The first detection of the [NII] 122 µm line from a high redshift galaxy was reported in this article, where the line was strongly (> 6 µm) detected from SMMJ02399-0136, and H1413+117 (the Cloverleaf QSO) using the Redshift(z) and Early Universe Spectrometer (ZEUS) on the CSO.