2010PASP..122..379T


Query : 2010PASP..122..379T

2010PASP..122..379T - Publ. Astron. Soc. Pac., 122, 379-395 (2010/April-0)

Spectral energy distributions of Be and other massive stars.

TOUHAMI Y., RICHARDSON N.D., GIES D.R., SCHAEFER G.H., BOYAJIAN T.S., WILLIAMS S.J., GRUNDSTROM E.D., McSWAIN M.V., CLEMENS D.P. and TAYLOR B.

Abstract (from CDS):

We present spectrophotometric data from 0.4 µm to 4.2 µm for bright, northern sky, Be stars and several other types of massive stars. Our goal is to use these data with ongoing high-angular-resolution interferometric observations to model the density structure and sky orientation of the gas surrounding these stars. We also present a montage of the Hα and near-infrared emission lines that form in Be star disks. We find that a simplified measurement of the IR excess flux appears to be correlated with the strength of emission lines from high level transitions of hydrogen. This suggests that the near-IR continuum and upper level line fluxes both form in the inner part of the disk, close to the star.

Abstract Copyright: ∼

Journal keyword(s): Stars

Errata: Addendum PASP vol. 124, p. 515 (2012)

Simbad objects: 41

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Number of rows : 41
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 1561 * 00 20 05.1661061352 +48 51 55.615971024 6.600 6.560 6.530     A0Vs 44 0
2 * omi Cas Be* 00 44 43.5186007265 +48 17 03.731037403 3.91 4.44 4.50 4.45 4.50 B5IIIe 291 0
3 * gam Cas HXB 00 56 42.5310945 +60 43 00.264089 1.18 2.29 2.39 2.32 2.40 B0.5IVpe 1253 0
4 * phi Per Be* 01 43 39.6379691568 +50 41 19.433124998 3.10 4.02 4.06 3.90 3.88 B1.5V:e-shell 594 0
5 HD 11946 * 01 59 38.0376593064 +64 37 17.760134928   5.273 5.278     A0Vn 68 0
6 HD 19600 PM* 03 10 08.8395959400 +27 49 11.157358944   6.427 6.412     A0V 63 0
7 * psi Per Be* 03 36 29.3797327450 +48 11 33.484405927 3.60 4.17 4.23     B5Ve 431 0
8 HD 23258 * 03 44 28.2037966608 +20 55 43.448620908   6.100 6.074     A0Vp_lB 60 0
9 * eta Tau Be* 03 47 29.0765529 +24 06 18.488347 2.44 2.78 2.87 2.84 2.88 B7III 557 1
10 * 28 Tau Be* 03 49 11.2165977912 +24 08 12.156712008 4.73 5.01 5.09   5.08 B8Vne 494 0
11 V* X Per HXB 03 55 23.0777456088 +31 02 45.039836148 6.090 6.840 6.720     O9.5III 1037 0
12 HD 25152 * 04 01 14.8307127768 +36 59 22.121343888 8.18 6.387 6.389     A0V 50 0
13 * c Per Be* 04 08 39.6935695869 +47 42 45.038007366 3.45 4.00 4.03 3.91 3.93 B3Ve 394 0
14 HD 29526 PM* 04 41 24.1285097472 +48 18 03.165290280   5.642 5.652     A0V 66 0
15 * 18 Ori * 05 16 04.1346616440 +11 20 28.878184140   5.500 5.515     A0V 73 0
16 * eps Ori s*b 05 36 12.81335 -01 12 06.9089 0.48 1.51 1.69 1.76 1.93 B0Ia 921 0
17 * zet Tau Be* 05 37 38.6854231 +21 08 33.158804 2.22 2.84 3.03 3.06 3.15 B1IVe_shell 751 0
18 * zet Ori ** 05 40 45.52666 -01 56 33.2649 0.50 1.56 1.77 1.85 2.05 O9.7Ib+B0III 375 0
19 * zet Ori A SB* 05 40 45.527143 -01 56 33.26036   1.79 1.90     O9.2IbvarNwk 680 0
20 * kap Ori s*b 05 47 45.3888404 -09 40 10.577707 0.87 1.88 2.06 2.09 2.27 B0.5Ia 588 0
21 HD 45380 * 06 26 44.8518087216 -07 30 42.985244628   6.29 6.33     B9V 54 0
22 * bet CMi Be* 07 27 09.0417373 +08 17 21.536745 2.52 2.80 2.89 2.90 2.96 B8Ve 400 0
23 * del03 CMi * 07 34 15.8926031424 +03 22 18.207554880   5.789 5.817     B9V 62 0
24 * 50 Lib HB* 16 00 47.6323225512 -08 24 40.889775888   5.557 5.526     A0V 87 0
25 * zet Oph Be* 16 37 09.5400587698 -10 34 01.509742704 1.73 2.58 2.56 2.46 2.50 O9.2IVnn 1908 0
26 * ups Sgr Be* 19 21 43.6225957281 -15 57 18.062726294 4.18 4.71 4.61 4.34 4.21 B2Vp_sh 312 0
27 HD 182678 SB* 19 26 24.5750707560 -14 33 04.374423360   6.734 6.694     A0V 41 0
28 * b02 Cyg Be* 20 09 25.6190611128 +36 50 22.633958400 4.03 4.80 4.93     B2.5Ve 281 0
29 HD 192538 * 20 14 04.8813535248 +36 36 17.578013580   6.448 6.464     A0V 76 0
30 * P Cyg s*b 20 17 47.2019733389 +38 01 58.549132671 4.66 5.24 4.82 4.28 4.02 B1-2Ia-0ep 1200 1
31 * f01 Cyg Be* 20 59 49.5541247496 +47 31 15.363746436 3.77 4.71 4.75 4.62 4.63 B1.5Vnne 514 0
32 * ups Cyg Be* 21 17 55.0858548408 +34 53 48.825463560 3.50 4.32 4.42 4.37 4.45 B2Vne 321 0
33 HD 205314 ** 21 32 56.5920346080 +49 58 39.478477980   5.721 5.755     A0V 73 0
34 * 79 Cyg * 21 43 25.6523360208 +38 17 00.927883932   5.688 5.695     A0V 50 0
35 * omi Aqr Be* 22 03 18.8440617830 -02 09 19.313835540 4.22 4.64 4.69 4.70 4.74 B5V 279 0
36 * 31 Peg Be* 22 21 31.0751048 +12 12 18.662815 4.08 4.89 4.99 5.06 5.20 B3III 227 0
37 * gam Aqr PM* 22 21 39.3715681296 -01 23 14.457098796 3.65 3.791 3.834     A0V 180 0
38 * pi. Aqr Be* 22 25 16.6230017410 +01 22 38.634449478 3.64 4.60 4.64 4.48 4.48 B1III-IVe 436 0
39 * bet Psc Be* 23 03 52.6132153632 +03 49 12.164302217 3.90 4.40 4.52 4.54 4.67 B6Ve 259 0
40 HD 223386 PM* 23 48 53.9708557608 +59 58 44.242748796   6.311 6.324     A0V 59 0
41 * rho Cas LP* 23 54 23.0325302520 +57 29 57.774737400 7.00 5.85 4.59 3.63 2.89 G2_0 401 0

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