No CrossRef data available.
Article contents
Fine structure of molecular clouds within 1 minute of arc of the Galactic Center
Published online by Cambridge University Press: 04 August 2017
Extract
We have observed the HCN(J=1–0) line in the vicinity of the galactic center with the 18″ beam of the Nobeyama 45-m telescope. Profiles were taken at 53 points within 1 arcmin from the galactic nucleus [R.A. = 17h42m29.29s, Dec. = −28°59′17.6″ (1950)] with a 10″ grid (see figure 1). A SSB cooled-mixer receiver (TRX = 600 K) and a wideband AOS (acousto-optical radiospectrometer) with 250 kHz resolution were used.
- Type
- PART II: COMPOSITION, STRUCTURE AND KINEMATICS
- Information
- Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 367 - 370
- Copyright
- Copyright © Reidel 1985