Details on Acronym: IRS | |
| IRS | (IR Source) |
| ***** | Avoid the usage of IRS, prefer [WKM94] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: PS | |
| PS | (Polarimetric Source) |
| ***** | Avoid the usage of PS, prefer [WKM94] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [WKM94] | |
| [WKM94] | (Weintraub+Kastner+Mahesh, 1994)= (IRS) = (PS) |
| Write: | <<[WKM94] IRS N>> <<[WKM94] PS N>> |
| N: | 9+1 |
| Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
| Note: | 1st ref.: N=5 sources 'IRS N' and N=1 Polarimetric Source 'PS 1'. 2nd ref.: Sources 'IRS N' (Nos 6-9) added |
| in source: | NGC 7129 |
| Ref: | =1994ApJ...420L..87W |
| by | WEINTRAUB D.A. , KASTNER J.H., MAHESH A. |
| Astrophys. J., 420, 87-90 (1994) | |
| Discovery of a deeply embedded companion to LkH-α 234. | |
| o | Table 1: <[WKM94] IRS N> (Nos 1-5), <[WKM94] PS 1> |
| Ref: | =1996ApJ...468L..45W |
| by | WEINTRAUB D.A. , KASTNER J.H., GATLEY I., MERRILL K.M. |
| Astrophys. J., 468, 45-50 (1996) | |
| Diffraction-limited 3.8 micron imaging of protostellar outflow sources. | |
| o | WK 34 = [WK96] 34, VLA 3 = [ARG94] VLA 3 |
| o | Table 1: <[WKM94] IRS N> (Nos 6-9) are new. Table 2: <[WKG96] DLIRIM N> (Nos 1-4) |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |