Details on Acronym: [RRN96] | |
[RRN96] | (Roddier+Roddier+Northcott+, 1996) |
Write: | <<[RRN96] GG Tau A>> <<[RRN96] GG Tau a>> <<[RRN96] GG Tau Aa>> |
N: | 6 |
Object: | * + ** (SIMBAD class: Star) |
Note: | GG Tau is composed of 4 stellar components: A.-brighter component of the close (north) binary (0"25 separation). a.-fainter component of the close (north) binary (0"25 separation). B.-brighter component of the south binary (1"4 separation) b.-fainter component of the south binary (1"4 separation) Aa.- north binary. Bb.- south binary (= CoKu GG Tau c) |
in source: | V* GG Tau |
Ref: | =1996ApJ...463..326R |
by | RODDIER C. , RODDIER F., NORTHCOTT M.J., GRAVES J.E., JIM K. |
Astrophys. J., 463, 326-335 (1996) | |
Adaptive optics imaging of GG Tauri: optical detection of the circumbinary ring. | |
o | <[RRN96] GG Tau A> (Nos A-B), <[RRN96] GG Tau a> (Nos a-b), <[RRN96] GG Tau Aa> (Nos Aa, Bb). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |