Gas‐Phase Polycyclic Aromatic Hydrocarbons in Absorption toward Protostellar Sources?
Authors:
- Jesse D. BregmanJBJesse D. Bregman
- Pasquale TemiPTPasquale Temi
- 10 June 2001
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 554 (1) , 126-131
Abstract
No abstract availableThis publication has 21 references indexed in Scilit:
- Search for NH3ice in cold dust envelopes around YSOsAstronomy & Astrophysics, 2001
- Discovery of the 11.2 Micron Polycyclic Aromatic Hydrocarbon Band in Absorption toward Monoceros R2 IRS 3The Astrophysical Journal, 2000
- New 3 Micron Spectra of Young Stellar Objects with H2O Ice BandsThe Astrophysical Journal, 1999
- Detection and Characterization of Cold Interstellar Dust and Polycyclic Aromatic Hydrocarbon Emission, fromCOBEObservationsThe Astrophysical Journal, 1997
- The Abundance of Interstellar CarbonThe Astrophysical Journal, 1996
- A Study of Absorption Features in the 3 Micron Spectra of Molecular Cloud Sources with H 2O Ice BandsThe Astrophysical Journal, 1996
- 10 micron spectroscopy of younger stars in the rho Ophiuchi cloudThe Astrophysical Journal, 1995
- Infrared spectroscopy of dense clouds in the C-H stretch region - Methanol and 'diamonds'The Astrophysical Journal, 1992
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- A survey of interstellar H I from L-alpha absorption measurements. IIThe Astrophysical Journal, 1978