Details on Acronym: [MSR2020] | |
| [MSR2020] | (Minniti+Sbordone+Rojas-Arriagada+, 2020) |
| Write: | <<[MSR2020] BNN>> <<[MSR2020] DNN>> |
| N: | 24+21 |
| Object: | Poss. Cepheid (SIMBAD class: Cepheid_Candidate = Cepheid Variable Candidate) |
| Stat: | is completely incorporated in Simbad |
| Note: | VLT X-Shooter observations of N=24+21 Cepheid candidates in the Galactic bulge area (-10°<l<+10°) and the disk area (l←10°) respectively. Use of VISTA Variables in the Via Lactea (VVV) Survey data. |
| Ref: | =2020A&A...640A..92M |
| by | MINNITI J.H. , SBORDONE L., ROJAS-ARRIAGADA A., ZOCCALI M., CONTRERAS RAMOS R., MINNITI D., MARCONI M., BRAGA V.F., CATELAN M., DUFFAU S., GIEREN W., VALCARCE A.A.R. |
| Astron. Astrophys., 640A, 92-92 (2020) | |
| Using classical Cepheids to study the far side of the Milky Way disk. I. Spectroscopic classification and the metallicity gradient. | |
| o | Tables 1+3: <[MSR2020] BNN> (Nos B01-B24). Tables 2+4: <[MSR2020] DNN> (Nos D01-D21). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |