Details on Acronym: ST | |
ST | (Sandage+Tammann, 1974) |
***** | Avoid the usage of ST, prefer [ST74b] |
Origin | of the Acronym: L (1988ApJ...334..144K) |
Details on Acronym: [ST74b] | |
[ST74b] | (Sandage+Tammann, 1974)= (ST) |
Write: | <<[ST74b] NGC NNNN A>> <<[ST74b] NGC NNNN NN>> <<[ST74b] NGC NNNN BNN>> <<[ST74b] IC 2574 A>> <<[ST74b] IC 2574 NN>> <<[ST74b] IC 2574 BNN>> <<[ST74b] Ho II A>> <<[ST74b] Ho II NN>> <<[ST74b] Ho II BNN>> <<[ST74b] Ho II RNN>> <<[ST74b] Ho I NN>> <<[ST74b] Ho I BNN>> |
N: | 244 |
Object: | * in G (SIMBAD class: Star) |
Note: | Format 'A': photoelectric sequence stars Format 'NN': secondary sequence stars Format 'BNN': Blue stars Format 'RNN': Red stars |
in source: | NGC 2366 |
in source: | IC 2574 /bin/bash: line 1: :w: command not found |
in source: | Holmberg II = DDO 50 |
in source: | NGC 4236 |
Ref: | =1974ApJ...191..603S |
by | SANDAGE A. , TAMMANN G.A. |
Astrophys. J., 191, 603-621 (1974) | |
Steps towards the Hubble constant. II. The brightest stars in late-type spiral galaxies. | |
o | Tables 1-7: <[ST74b] NGC 2366 A> (Nos A-I). <[ST74b] NGC 2366 NN> (Nos 1-30). <[ST74b] NGC 2366 BNN> (Nos B1-B28). <[ST74b] IC 2574 A> (Nos A-J). <[ST74b] IC 2574 NN> (Nos 1-20). <[ST74b] IC 2574 BNN> (Nos B1-B20). <[ST74b] Ho II A> (Nos A-J). <[ST74b] Ho II NN> (Nos 1-28). <[ST74b] Ho II BNN> (Nos B1-B31). <[ST74b] Ho II RNN> (Nos R1-R10). <[ST74b] Ho I NN> (Nos 1-10). <[ST74b] Ho I BNN> (Nos B1-B12). <[ST74b] NGC 4236 N> (Nos 1-8). <[ST74b] NGC 4236 BNN> (Nos B1-B18) |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |