Published November 15, 1985
| Version v1
Journal article
CO emission structure in the Taurus molecular cloud complex
Creators
- 1. Research Laboratory of Electronics and Department of Physics, Massachusetts Institute of Technology
Description
A survey of the J = 1 → 0 2.6 mm transition of CO covering 11.5 deg2 toward the Taurus dark cloud complex reveals three indications of systematic velocity structure:
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 298
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 818-826
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17042126
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON MONOXIDE; EMISSION; ENERGY-LEVEL TRANSITIONS; INTERSTELLAR GRAINS; MAPS; MASS; NEBULAE; STELLAR WINDS; T TAURI STARS
- Descriptors DEC
- BINARY STARS; CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; ERUPTIVE VARIABLE STARS; OXIDES; OXYGEN COMPOUNDS; PARTICLES; STARS; STELLAR ACTIVITY; VARIABLE STARS