Difference between revisions of "B Stars"
From Telescope
Line 7: | Line 7: | ||
14 12 15.8043 | 14 12 15.8043 | ||
− | + | 02 24 33.958 | |
− | B 4.89 | + | B = 4.89 |
− | V 5.01 | + | |
+ | V = 5.01 | ||
A0Vp | A0Vp |
Revision as of 23:08, 14 June 2009
Summertime targets from Rich Townsend (June 2009) Ap/Bp stars - chemically peculiar with strong magnetic fields
CU Vir (HD 124224) -- short period, quite bright, the best-known 'stellar pulsar' (main sequence star with ~0.5d pulsed radio emission).
14 12 15.8043
02 24 33.958
B = 4.89
V = 5.01
A0Vp
V 2052 Oph (163472), which is a combination beta Cep/He-strong B2 star with a 3.64d period. Again, quite bright.
17 56 18.4009
+00 40 13.277
B 5.883 V 5.834
B2IV-V
V 1671 Cyg (HD 184927), which is a bit dimmer, and has a longer period, but appears to have a very oblique, strong field (seen from near pole on).
19 35 32.0099
+31 16 35.926
B 7.29 V 7.44
B2V