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Fine structure of molecular clouds within 1 minute of arc of the Galactic Center

Published online by Cambridge University Press:  04 August 2017

Norio Kaifu ,
Junji Inatani ,
Tesuo Hasegawa  and
Masaki Morimoto
Norio Kaifu
Affiliation:
Nobeyama Radio Observatory, Tokyo Astronomical Observatory
Junji Inatani
Affiliation:
Nobeyama Radio Observatory, Tokyo Astronomical Observatory
Tesuo Hasegawa
Affiliation:
Nobeyama Radio Observatory, Tokyo Astronomical Observatory
Masaki Morimoto
Affiliation:
Nobeyama Radio Observatory, Tokyo Astronomical Observatory

Extract

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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 

References

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