1997PASP..109..633D

Query : 1997PASP..109..633D

1997PASP..109..633D - Publ. Astron. Soc. Pac., 109, 633-638 (1997/June-0)

A photometric system for detection of embedded Wolf-Rayet stars.

DAMINELI A., JABLONSKI F., DE FREITAS L.C. and DE FREITAS PACHECO J.A.

Abstract (from CDS):

We describe a photometric system designed for detection of WR stars in the near infrared region and based on a combination of narrow band filters and a CCD detector. The system is sensitive to Of and faint lined WN and WC stars and suitable for obscured regions of star formation in our Galaxy.

Abstract Copyright: ∼

Journal keyword(s): Stars

Simbad objects: 30

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Number of rows : 30
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 RMC 135 WR* 05 38 33.6193296576 -69 04 50.510501688   12.63 13.48     WN7h+OB 63 0
2 Brey 81 WR* 05 38 36.4071127800 -69 06 57.534295248   14.02 13.76   12.80 WN8 41 0
3 Brey 79 WR* 05 38 39.1442162640 -69 06 21.297619692     13.5 13.33   WN6 39 0
4 Cl* NGC 2070 MH 57 s*b 05 38 40.2160044288 -69 05 59.915264352   12.97 13.0   12.91 O3If*/WN6-A 46 1
5 Brey 75 WR* 05 38 40.53 -69 05 57.2   12.84 12.75   12.34 WN6h 66 0
6 RMC 140a WR* 05 38 41.5967462055 -69 05 13.457120148   12.18 12.12   12.40 WN4+WC5 41 0
7 RMC 140b WR* 05 38 41.6202115352 -69 05 15.192382434   12.61 12.66   12.54 WN6 36 0
8 Brey 76 WR* 05 38 41.8800 -69 06 13.680     12.5     O2If*/WN5 34 1
9 Brey 77 WR* 05 38 42.1044150840 -69 05 55.335965424     12.86   12.79 O2If* 90 0
10 RMC 139 WR* 05 38 42.3537501576 -69 04 58.196699796   12.04 11.94     O6.5Iafc+O6Iaf 101 0
11 Cl* NGC 2070 MH 716 * 05 38 43.0737 -69 06 11.255   14.40 14.26   14.10 O2-4.5 22 0
12 BAT99 113 WR* 05 38 43.0917715292 -69 05 46.903118899   13.56 13.47   13.44 O2If*/WN5 53 0
13 Brey 83 WR* 05 38 44.0630210280 -69 05 55.683258756           WC4 27 0
14 Brey 84 HXB 05 38 44.2508644296 -69 06 06.004573020     13.10   12.70 WN5h:a 77 0
15 HD 269928 WR* 05 38 57.0667692816 -69 06 05.660419140   12.02 11.94 12.00 11.58 WN6/7 143 0
16 V* R Leo Mi* 09 47 33.4839808805 +11 25 43.823283729 9.22 8.94 7.53 3.39 0.12 M7-9e 943 1
17 V* U Hya C* 10 37 33.2729535 -13 23 04.352923 13.29 7.51 4.82 3.05 1.78 C-N5 314 0
18 * eta Car s*b 10 45 03.545808 -59 41 03.95124 6.37 7.03 6.48 6.123 4.41 LBV 2543 0
19 HD 96548 WR* 11 06 17.2032351624 -65 30 35.241182028 7.10 7.80 7.70 8.49   WN8h 427 0
20 HD 104994 WR* 12 05 18.7204232424 -62 03 10.140656832 9.95 10.94 10.93 11.03   WN3p-w 170 0
21 * tet Vir ** 13 09 56.9889385680 -05 32 20.414634792   4.385 4.397     A1IVs 277 0
22 HD 119078 WR* 13 43 16.3587374232 -67 24 04.973391360 9.11 9.737 9.40 10.08   WC7/8 110 0
23 * 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
24 HD 151932 WR* 16 52 19.2477039480 -41 51 16.270066224 6.06 6.79 6.51 7.64   WN7h 326 0
25 HD 152408 WR* 16 54 58.5051071856 -41 09 03.093075612 5.17 5.92 5.77 7.00   O8Iape 388 0
26 HD 164270 WR* 18 01 43.1453595672 -32 42 55.161329040 8.52 8.97 8.74 9.51   WC9d+? 233 0
27 HD 165763 WR* 18 08 28.4692108104 -21 15 11.183076540 7.16 7.54 7.82 8.55   WC6 286 0
28 * lam Sgr PM* 18 27 58.2407185 -25 25 18.114589 4.75 3.85 2.81 2.06 1.50 K1IIIb 290 0
29 V* RR Tel Sy* 20 04 18.5404499712 -55 43 33.153979080 9.93 11.33 10.81 11.689   M5e 550 0
30 NGC 7009 PN 21 04 10.8155187648 -11 21 48.580157556   12.48 12.07     ~ 1020 1

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