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Survey of Molecular Lines Near the Galactic Center. III. 6-Centimeter Formaldehyde Absorption at b = -2' from ℓ = 2°.0 to ℓ = 4°.5 and at b = -12' from ℓ = 358°.5 to ℓ = 2°.0

Scoville, N. Z. and Solomon, P. M. (1973) Survey of Molecular Lines Near the Galactic Center. III. 6-Centimeter Formaldehyde Absorption at b = -2' from ℓ = 2°.0 to ℓ = 4°.5 and at b = -12' from ℓ = 358°.5 to ℓ = 2°.0. Astrophysical Journal, 180 . pp. 55-59. ISSN 0004-637X. doi:10.1086/151941. https://resolver.caltech.edu/CaltechAUTHORS:20190329-150046925

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Abstract

Our initial survey in the 6-cm transition of formaldehyde near the galactic plane (b = -2') has been extended out to ℓ = 4°.5, and a parallel strip at b = -12' has been mapped between ℓ = 358°.5 and 2°.0. These new observations suggest that the group of dense, low-positive-velocity clouds does not continue beyond ℓ = 2° and that the negative-velocity clouds are part of an arm structure within 300 pc of the galactic center and having a total mass of ~10^6 M_⊙. We also note the existence of molecular gas at ℓ = 2°.3 with a velocity of 240 km s^(-1) (similar to that of H I in the rotating nuclear disk).


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/151941DOIArticle
http://adsabs.harvard.edu/abs/1973ApJ...180...55SADSArticle
ORCID:
AuthorORCID
Scoville, N. Z.0000-0002-0438-3323
Additional Information:© 1973. The American Astronomical Society.
Subject Keywords:molecules - galactic structure - galactic nuclei
DOI:10.1086/151941
Record Number:CaltechAUTHORS:20190329-150046925
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190329-150046925
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:94299
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:29 Mar 2019 22:53
Last Modified:16 Nov 2021 17:04

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