1999A&A...344..614H


Query : 1999A&A...344..614H

1999A&A...344..614H - Astronomy and Astrophysics, volume 344, 614-616 (1999/4-2)

Emission line star 3G 71: a Herbig Ae/Be star candidate.

HANG H.-R., LIU Q.-Z. and XIA J.-P.

Abstract (from CDS):

We present new optical spectral observations of 3G 71, the previously suspected optical counterpart of the hard X-ray source 1H 2214+589. The spectra of 3G 71 exhibit many forbidden lines, unusually intense H-Balmer emission lines and the approximately B5 spectral type. Such spectral features, together with its large IRAS infrared color excess and associated with nebulosity, provide evidences that the star may be a Herbig Ae/Be star candidate rather than the optical counterpart of Be/X-ray source of 1H 2214+589.

Abstract Copyright:

Journal keyword(s): stars: individual: 3G 71 - stars: pre-main sequence

CDS comments: 3G 71 = EM* GGR 71

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 WRAY 15-793 HXB 11 20 57.1736884968 -61 55 00.166078020 12.81 13.06 12.12     O9.5III/Ve 182 0
2 HD 100546 Be* 11 33 25.4408872296 -70 11 41.241297948   6.71 6.30   6.64 A0VaekB8_lB 717 1
3 V* DX Cha Ae* 12 00 05.0868602544 -78 11 34.565724312   6.81 6.60     A0_sh 321 0
4 EM* GGR 71 Em* 22 26 38.7333592272 +61 13 31.568432916   13.55 12.47     B[e] 27 0
5 4U 2238+60 HXB 22 39 20.8443538152 +61 16 26.607472284   16.26 14.80 13.89 12.92 Be 46 0

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