Details on Acronym: [SGK2020] | |
[SGK2020] | (Saha+Gopinathan+Kamath+, 2020) |
Write: | <<[SGK2020] NN>> <<[SGK2020] 13b>> <<[SGK2020] cNN>> <<[SGK2020] xN>> <<[SGK2020] PNN>> |
N: | 58+1+20+5+11 |
Object: | Poss. YSO + Comoving Source + (X) + Column Density Peak (SIMBAD class: Unknown = Object of Unknown Nature) |
Note: | ARIES 104cm Sampurnanand telescope AIMPOL polarimetry and Himalayan Chandra 2m telescope (HCT, India) HFOSC observations of N=59 YSO candidates and N=20 comoving sources in the field of HD 200775. N=5 X-ray sources, using the XMM-Serendipitous Source Catalog N=11 column density peaks, identified on a Herschel SPIRE 250µm image. Use of Gaia DR2, Spitzer, 2MASS, and WISE data. |
Ref: | =2020MNRAS.494.5851S |
by | SAHA P. , GOPINATHAN M., KAMATH U., LEE C.W., PURAVANKARA M., MATHEW B., SHARMA E. |
Mon. Not. R. Astron. Soc., 494, 5851-5871 (2020) | |
A census of young stellar population associated with the Herbig Be star HD 200775. | |
o | Tables 3+7: <[SGK2020] NNa> (Nos 1-13, 13b, 14-58). Table 4: <[SGK2020] cNN> (Nos c1-c20). Table 5: <[SGK2020] xN> (Nos x1-x5). Fig. 17: <[SGK2020] PNN> (Nos P1-P11). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |