Herbig Ae/Be
stars
Herbig Ae/Be stars (so called Herbig-Bell)
are young object of spectral type A or earlier, with emission lines,
located in an obscured region of the sky and illuminates fairly
bright nebulosity in its immediate vicinity (star forming regions).
Many of this pre-main sequence stars are located
on the Orion nebula. Note that T Tauri type stars are low-mass counterparts
of higher-mass Herbig Ae/Be stars. Fu Orionis stars can be also
likened to the Herbig Ae/Be class.
Often, the only difference between the Ae/Be
stars and the Herbig Ae/Be stars comes from the presence of the
association with nebulosity for the last situation. Generaly, the
emission concern H-alpha and Ca II H&K lines.
The most bright Herbig-Bell stars:
HD Name
R.A.
Dec. Mv Spec.
275877 XY
Per 3 h 46.6 38°
59 9.36 A5:e T
Tau 4 h 21.9 19°
32 9.90 K0IV, V(Li) 283572 4
h 21.9 28° 18 9.04 G5
IV(Li) 283571 RY Tau 4
h 21.9 28° 27 10.0 KAIV,
V(Li) 31293 AB Aur 4
h 55.7 30° 33 7.07 B9,
A+e+shl 282624 SU Aur 4
h 56.0 30° 34 8.93 G2
III(Li) UX
Ori 5 h 04.5 -03°
48 9.72 A3e III RW
Aur A 5 h 07.8 30°
24 10.1 K1: CO
Ori 5 h 27.6 11°
26 9.83 F8:e V(Li) 244138 GW
Ori 5 h 29.1 11°
52 9.80 G5 (Li) 245059 5
h 34.6 10° 07 9.82 K3
V:(Li) 245185 5
h 35.1 10° 02 9.93 A5e
NV Ori
5 h 35.5 -05°
33 9.91 F4, 8 III,V MX
Ori 5 h 35.6 -05°
09 9.90 G2(Li) T
Ori 5 h 35.8 -05°
29 9.96 A3e 36910 CQ
Tau 5 h 35.9 24°
44 10.0 A8ve 245465 BN
Ori 5 h 36.5 06°
50 9.64 F2,3e V380
Ori 5 h 36.8 -06° 40 10.0
A1:e V586
Ori 5 h 37.0 -06° 09 9.54
A2e FU
Ori 5 h 45.6 09°
04 9.24 G; I, II 288313 5
h 54.1 01° 40 9.93 K2:n(Li)
250550 MCW 789 6
h 02.0 16° 31 9.48 B9eq
259431 MCW 147 6
h 33.1 10° 19 8.69 B5:e
53179 Z CMa 7
h 03.7 -11° 33 9.35 B?eq
pec 144668 V856 Sco 16 h
08.6 -39° 06 6.79 A7e
III,IV 200775 MCW 361 21
h 01.6 68° 10 7.39 A0pe+shell
152404 AK Sco 16
h 54.7 -36° 53 8.82 F5e
+41°3731
20 h 24.3 42° 18 9.88
B2, 3e +46°
3471 21 h 52.6 47° 14 10.1
A4:e+shell
Click here for a complete
catalog of Herbig-Bell stars (http://www-astro.phast.umass.edu/catalogs/HBC/HBC.html) |