2003A&A...410..199D


Query : 2003A&A...410..199D

2003A&A...410..199D - Astronomy and Astrophysics, volume 410199-216 (2003/10-4)

A quest for PMS candidate stars at low metallicity: Variable HAe/Be and Be stars in the Small Magellanic Cloud.

DE WIT W.J., BEAULIEU J.-P., LAMERS H.J.G.L.M., LESQUOY E. and MARQUETTE J.-B.

Abstract (from CDS):

We report the discovery of 5 new Herbig Ae/Be candidate stars in the Small Magellanic Cloud in addition to the 2 reported in Beaulieu et al. (2001A&A...380..168B). We discuss these 7 HAeBe candidate stars in terms of (1) their irregular photometric variability, (2) their near infrared emission, (3) their Hα emission and (4) their spectral type. One star has the typical photometric behaviour that is observed only among Pre-Main Sequence UXOrionis type stars. The objects are more luminous than Galactic HAeBe stars and Large Magellanic Cloud HAeBe candidates of the same spectral type. The stars were discovered in a systematic search for variable stars in a subset of the EROS2 database consisting of 115612 stars in a field of 24x24-arcmin in the Small Magellanic Cloud. In total we discovered 504 variable stars. After classifying the different objects according to their type of variability, we concentrate on 7 blue objects with irregular photometric behaviour. We cross-identified these objects with emission line catalogues from Simbad and JHK photometry from 2MASS. The analysis is supplemented with obtained narrow and broad band imaging. We discuss their variability in terms of dust obscuration and bound-free and free-free emission. We estimate the influence of metallicity on the circumstellar dust emission from pre-main sequence stars.

Abstract Copyright: ∼

Journal keyword(s): stars: early type - stars: formation - stars: pre-main sequence - Be stars - stars: variables: SMC

Nomenclature: Table 3: ESHC N (Nos 3-7) added.

Simbad objects: 18

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Number of rows : 18
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 [MA93] 535 LP* 00 52 06.4352475288 -73 06 29.486617956   14.2 13.983   13.72 ~ 8 0
2 [MA93] 563 Em* 00 52 21.5589541512 -73 13 32.265278616   17.4 16.6 16.9 16.84 ~ 5 0
3 OGLE J005232.63-731707.2 Y*O 00 52 32.6432337336 -73 17 07.719708408   16.957 17.012   16.946 B2IV-V 6 0
4 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
5 [MA93] 619 Em* 00 52 52.5102923520 -73 18 34.016070996   15.417 15.254   14.684 B?e 10 0
6 LIN 232 Y*O 00 53 02.7894270720 -73 17 59.597977668   15.072 15.079   14.947 B4IIIe 9 0
7 2MASS J00535674-7310293 Y*O 00 53 56.7756447240 -73 10 29.528474016   14.901 15.049   14.865 ~ 5 0
8 LIN 264 Em* 00 54 37.5734143296 -73 04 56.885683296   15.128 15.177   15.066 ~ 7 0
9 * ome Ori Be* 05 39 11.1457980782 +04 07 17.288290296 3.73 4.48 4.59 4.57 4.67 B3Ve 424 1
10 EM* MWC 137 Ae* 06 18 45.5220873216 +15 16 52.244494608 12.89 13.30 13.759 11.67 10.31 sgB[e]d 259 1
11 HD 259431 Ae* 06 33 05.1906369144 +10 19 19.982565336 8.39 8.95 8.72     B6ep 299 1
12 * kap CMa Be* 06 49 50.4591124672 -32 30 30.523820933 2.73 3.68 3.89 3.91 4.05 B1.5Ve 298 0
13 HD 52721 Ae* 07 01 49.50977 -11 18 03.3219 5.88 6.65 6.59 7.52   B2Vne 230 0
14 EM* LkHA 218 Ae* 07 02 42.5309892768 -11 26 11.826714804   13 11.63     A0e 70 0
15 HD 53367 Ae* 07 04 25.5189757244 -10 27 15.613478141 6.81 7.40 6.96 7.92   B0IV/Ve 330 0
16 HD 76534 Be* 08 55 08.70673 -43 27 59.8852 7.04 7.62 7.50 8.94   B2Vn 142 0
17 HD 150193 Ae* 16 40 17.9243127240 -23 53 45.193372692 9.69 9.32 8.79 8.41   A3Va(e) 336 0
18 HD 200775 Ae* 21 01 36.9205762896 +68 09 47.789578836 7.34 7.754 7.427 8.13   B2Ve 582 0

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