Étoiles Herbig de type Ae/Be
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)
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