Details on Acronym: HB | |
| HB | (Hawkins+Bessell) |
| ***** | Avoid the usage of HB, prefer [HB88] |
| Origin | of the Acronym: L = Found in the literature |
Details on Acronym: [HB88] | |
| [HB88] | (Hawkins+Bessell, 1988)= (HB) |
| Write: | <<[HB88] NN>> <<[HB88] {S|M|N}NN>> <<[HB88] HHMM+DDMM>> |
| N: | 37 |
| Object: | * (SIMBAD class: Star) |
| Note: | Table 3: N=14 * at SGP, among (Nos 5-36). Table 5: in the format, the letters S or M or N stands for spectral type. N=5 among (Nos S1-S6). N=8 among (Nos M1-M20), N=11 already studied in 1986MNRAS.223..845H. N=4 among (Nos N1-N7). |
| Ref: | =1988MNRAS.234..177H |
| by | HAWKINS M.R.S. , BESSELL M.S. |
| Mon. Not. R. Astron. Soc., 234, 177-191 (1988) | |
| The luminosity function for low mass stars. | |
| o | Table 3: <[HB88] NN> N=14 among (Nos 5-36), Table 5: <[HB88] ANN> N=5 among (Nos S1-S6), N=8 among (Nos M1-M20), N=4 among (Nos N1-N7) |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |