Constraints on the molecular properties of interstellar X-ogen derived from radio observations
Journal Article
·
· Astrophys. J., v. 200, no. 3, pp. 584-593
Twenty-eight X-ogen emission sources at 89.189 GHz have been detected and observed; of these, 20 are new X-ogen sources which also contain other interstellar molecules. No infrared stars were found to be X-ogen sources. A new rest frequency, 89,188.65 MHz, has been derived for X-ogen. We show that X- ogen is not SiC, C$sub 2$H, or any molecule with spin-doubling and/or hyperfine structure. (AIP)
- Research Organization:
- University of Virginia, Charlottesville
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-33-010173
- OSTI ID:
- 4123257
- Journal Information:
- Astrophys. J., v. 200, no. 3, pp. 584-593, Journal Name: Astrophys. J., v. 200, no. 3, pp. 584-593; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
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