Details on Acronym: [KPB2018] | |
[KPB2018] | (Kurtovic+Perez+Benisty+, 2018) |
Write: | <<[KPB2018] HT Lup A>> |
N: | 3 |
Object: | YSO (SIMBAD class: YSO = Young Stellar Object) |
Stat: | is completely incorporated in Simbad |
Note: | N=3 components in the triple stellar system V* HT Lup. Use of data from the Disk Substructures at High Angular Resolution Project (DSHARP). |
Ref: | =2018ApJ...869L..44K |
by | KURTOVIC N.T. , PEREZ L.M., BENISTY M., ZHU Z., ZHANG S., HUANG J., ANDREWS S.M., DULLEMOND C.P., ISELLA A., BAI X.-N., CARPENTER J.M., GUZMAN V.V., RICCI L., WILNER D.J. |
Astrophys. J., 869L, 44-44 (2018) | |
The Disk Substructures at High Angular Resolution Project (DSHARP). IV. Characterizing substructures and interactions in disks around multiple star systems. | |
o | Fig. 2, Table 1: <[KPB2018] HT Lup A> (Nos A-C). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |