Details on Acronym: [W89] | |
[W89] | (Wootten, 1989) |
Write: | <<[W89] AN>> <<[W89] Aa>> <<[W89] B>> |
N: | 2+2+2 |
Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
Stat: | is completely incorporated in Simbad |
Note: | N=2 radio-components associated with IRAS 16293-2422, (Nos A-B), No. A been resolved in 2 closely separated cm sources (A1 and A2). No. A have 2 smm components different from the cm ones (Aa and Ab). See also [MWW92], [LCR2007]. |
Ref: | =1989ApJ...337..858W |
by | WOOTTEN A. |
Astrophys. J., 337, 858-864 (1989) | |
The duplicity of IRAS 16293-2422 : a protobinary star ? | |
o | <[W89] A> (Nos A and B), <[W89] AN> (Nos A1 and A2) |
Ref: | =2005ApJ...632..371C |
by | CHANDLER C.J. , BROGAN C.L., SHIRLEY Y.L., LOINARD L. |
Astrophys. J., 632, 371-396 (2005) | |
IRAS 16293-2422: proper motions, jet precession, the hot core, and the unambiguous detection of infall. | |
o | Table 3: <[W89] Aa> (Nos Aa and Ab). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |