Details on Acronym: BW | |
| BW | (Baade's window) |
| ***** | Avoid the usage of BW, prefer [RT92] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: RT | |
| RT | (Ruelas-Mayorga+Teague) |
| ***** | Avoid the usage of RT, prefer [RT92] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [RT92] | |
| [RT92] | (Ruelas-Mayorga+Teague, 1992)= (BW) = (RT) |
| Write: | <<[RT92] FF-NN>> <<[RT92] N(FF-NN)>> <<[RT92] OUT N>> |
| N: | 578+8+2 |
| Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
| Note: | The authors use a format 'FF/NN' In the format, 'FF' stands for fields (Nos 1-31) Other formats 'N(FF-NN)' is for misidentified objects, and 'OUT N' for objects out of fields. See also [R91] and [RT93] |
| Ref: | =1992A&AS...93...61R |
| by | RUELAS-MAYORGA R.A. , TEAGUE P.F. |
| Astron. Astrophys., Suppl. Ser., 93, 61-86 (1992) | |
| Distribution and studies of the infrared stellar population in the galaxy. III. Baade's window photometry. | |
| o | Tables 1, 2: <[RT92] FF-NN> N=578, <[RT92] N(FF-NN) N=8, <[RT92] OUT N> (Nos 1-2) |
| =E= | Catalogue in electronic form as J/A+AS/93/61 |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |