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[vsnet-j 1159] Re: WR106 = HadV84

Re: [vsnet-j 1154] Re: WR106 = HadV84

> WR 113もけっこう深い(Veen et al.にあったやつ)

　CV Ser のデータです。IRASでそれほど明るくなく、結構スカスカで見えている
　のではないかと思います。

＃食変光星であることが敬遠されているのか(^^;)、VSNETには１件の報告もなし。

GSC5685.3986 181907.41 -113758.0 (2000.0)  9.36 0
USNO0750.12975194 181907.370 -113759.56 (2000.0)  8.8  9.4 *
USNO0750.12975217 181907.413 -113758.01 (2000.0)  9.4 99.9
181907.1 -113806 (2000.0) SD-11.4593 8.7
181907.2 -113758 (2000.0) LSIV-11.14 10.2p WC 
181906.4 -113754 (2000.0) V=9.138(-) b-y=0.293(-) m1=0.528(-) c1=-0.355(-) beta=2.652(-)
181907.2 -113758 (2000.0) SAO161325 99.9 8.8 Oa
181907.2 -113758 (2000.0) WR113 9.43 WC8+O8-9 CV Ser
181907.2 -113800 (2000.0) *CVSER
181907.4 -113800 (2000.0) UBV_CVSer 9.11 0.76 -0.24 .019 .029 .014 C8 N=2 Nm=7 -
181907.3 -113759 (2000.0) 908H 0.72 HIP089769 plx=1.38(1.32) (0.03 0.03)
181907.3 -113759 (2000.0) 918V
181907.3 -113758 (2000.0) 920 0.66 TYC2-5685.3986.1 (9.27 0.02) (10.05 0.03)
181907.4 -113757 (2000.0) SERCV * E/D/WR 9.00 9.63 V 40785.29 29.7005 - WC8+O8-O9III-IV R1/SER1

IRAS18162-1139 181616.9 -113910 (1950.0)
    F12=2.09  F25=2.75  F60=120.20L F100=630.87L
    VAR=95 LRS=-1
 possibly IIIa: variable star with more evolved O-rich c.s. shell
 or VIb: variable star with relatively hot dust close to
      the star and relatively cold dust at large distance
      may be O-rich
181904.3 -113752 (2000.0) IRAS18162-1139 2.168 2.820 117.900L 633.700L 95%
181904.3 -113752 (2000.0) SSC18162-1139 2.168 2.820 117.900L 633.700L

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