High Angular Resolution Observations of the (J, K) = (1, 1), (2, 2), and (3, 3) Transitions of Ammonia in NGC 253 | Zendy

Shuro Takano | Zendy; P. Höfner | Zendy; G. Winnewisser | Zendy; Naomasa Nakai | Zendy; Kentarou Kawaguchi | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

High Angular Resolution Observations of the (J, K) = (1, 1), (2, 2), and (3, 3) Transitions of Ammonia in NGC 253

Author(s) -

Shuro Takano,

P. Höfner,

G. Winnewisser,

Naomasa Nakai,

Kentarou Kawaguchi

Publication year - 2005

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/57.4.549

Subject(s) - physics , galaxy , astrophysics , ammonia , line (geometry) , prime (order theory) , galactic center , high resolution , center (category theory) , angular resolution (graph drawing) , equivalent width , star formation , bar (unit) , spectral line , astronomy , emission spectrum , geometry , crystallography , meteorology , remote sensing , chemistry , mathematics , organic chemistry , combinatorics , geology

The nearby starburst galaxy NGC 253 was mapped in the ammonia $(J, K) = (1, 1), (2, 2)$, and $(3, 3)$ lines in the 23 GHz region with the Very Large Array. The angular resolutions were about $4 {{}^{\prime \prime }} \times 3 {{}^{\prime \prime }}$. The distributions of the three lines were different from one another. The $(1, 1)$ and $(3, 3)$ lines were distributed along the bar mainly at the nort...

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research