Detection of high-excitation rotational lines of cyanoacetylene in the OMC 1 region
- 1. Millimeter Wave Observatory, Electrical Engineering Research Lab, The University of Texas at Austin, Austin, Texas
Description
Six new high-excitation transitions of cyanoacetylene (HC3N) lying between 209 and 282 GHz have been detected toward OMC 1. Line widths are approx.10 km s-1, broader than the low-frequency HC3N lines. Spectra of two low-frequency (82 and 91 GHz) HC3N transitions with a spatial resolution similar to that of the high-frequency transitions, show both the broad feature and the more commonly seen narrow component. While the low-frequency HC3N transitions are spatially extended in OMC 1, the broad component of the high-frequency HC3N transitions appears to be confined to an unresolved region of approx.1' or less. The intensities of the broad component are used to find the density and temperature of the broad-line-emitting region. The best fit to the HC3N line intensities yields T/sub K/ = 125 K and a density of > or =107 cm-3
Additional details
Publishing Information
- Journal Title
- Astrophys. J., Lett. Ed.
- Journal Volume
- 244
- Journal Issue
- 2
- Series
- Astrophys. J., Lett. Ed.
- Journal Page Range
- L107-L110
- ISSN
- 0571-7248
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 12630969
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ENERGY SPECTRA; ENERGY-LEVEL TRANSITIONS; EXCITED STATES; INTERSTELLAR SPACE; LINE WIDTHS; NEBULAE; NITRILES; ROTATIONAL STATES
- Descriptors DEC
- ENERGY LEVELS; ORGANIC COMPOUNDS; ORGANIC NITROGEN COMPOUNDS; SPACE; SPECTRA