Published May 1, 1987
| Version v1
Journal article
A dense molecular outflow in Orion B
Creators
- 1. Mullard Radio Astronomy Observatory, Cambridge (UK). Cavendish Lab.
Description
HCO+ J=3-2 maps with 60 arcsec resolution of Orion B are presented. A dense (approx.105 cm-3) component has been detected in the Orion B bipolar outflow. Our maps of the cloud core give evidence that the evolution of the outflow has been influenced by the local density gradients in the molecular cloud. A search has also been made for H2S(1) ν=1-0 emission along the outflow axis and an upper limit set. H2 emission was detected 80 arcsec east of the outflow centre. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 226
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 237-248
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 18078095
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- EXPERIMENTAL DATA; FORMYL RADICALS; GAS FLOW; GHZ RANGE 100-1000; HYDROGEN SULFIDES; INFRARED RADIATION; MAPS; MOLECULES; NEBULAE; RADIAL VELOCITY; RADIOWAVE RADIATION
- Descriptors DEC
- ACYL RADICALS; CHALCOGENIDES; DATA; ELECTROMAGNETIC RADIATION; FLUID FLOW; FREQUENCY RANGE; GHZ RANGE; HYDROGEN COMPOUNDS; INFORMATION; NUMERICAL DATA; RADIATIONS; RADICALS; SULFIDES; SULFUR COMPOUNDS; VELOCITY