us A. CO is detected in S1 and S2 corresponding to several HI and stellar shells (see [MQG83]). S3 is a series of pointing along an optical shell. S4 is a single pointing. Map in Fig.1. | |
in source: | Cen A = NGC 5128 |
Ref: | =2000A&A...356L...1C |
by | CHARMANDARIS V. , COMBES F., VAN DER HULST J.M. |
Astron. Astrophys., 356, 1-4 (2000) | |
First detection of molecular gas in the shells of Cen A. | |
o | Fig.1: <[CCV2000] SN> (Nos S1-S4). |
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