Details on Acronym: [DNM2003] | |
[DNM2003] | (De Breuck+Neri+Morganti+, 2003) |
Write: | <<[DNM2003] J2330+3927 a>> <<[DNM2003] J2330+3927 Star>> <<[DNM2003] J2330+3927 CO>> <<[DNM2003] J2330+3927 W>> |
N: | 3+1+1+3 |
Object: | Part of G + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature) |
Stat: | is completely incorporated in Simbad |
Note: | Multi-frequency study of the radio galaxy B3 2327+391. N=3 components (Nos a-c), N=1 Offset star in the field, N=1 CO peak, and N=3 radio components (Nos N, C, S). [DNM2003] J2330+3927 a is the most likely AGN position from optical/IR observations but it is not coincident with the central radio component. See also [PD2005] |
in source: | B3 2327+391 |
Ref: | =2003A&A...401..911D |
by | DE BREUCK C. , NERI R., MORGANTI R., OMONT A., ROCCA-VOLMERANGE B., STERN D., REULAND M., VAN BREUGEL W., ROETTGERING H., STANFORD S.A., SPINRAD H., VIGOTTI M., WRIGHT M. |
Astron. Astrophys., 401, 911-925 (2003) | |
CO emission and associated H I absorption from a massive gas reservoir surrounding the z = 3 radio galaxy B3 J2330+3927. | |
o | B3 J2330+3927 = B3 2327+391 in SIMBAD. 6C J1908+7220 (2000 coord.) = 6C 1909+7215 in SIMBAD. 8C 1425+635 is a misprint for 8C 1435+633. B3 J2330+3929 and J2330+3926 are misprint for B3 J2330+3927. |
o | Fig.2, Table 1: <[DNM2003] J2330+3927 a> (Nos a-c), <[DNM2003] J2330+3927 Star> N=1, <[DNM2003] J2330+3927 CO> N=1. Table 3: <[DNM2003] J2330+3927 W> (Nos N, C, S). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |