[vsnet-id 696] Re: [vsnet-chat 5544] The curious case of BD+59 224

[Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>]

Re: [vsnet-chat 5544] The curious case of BD+59 224

   The IRAS colors are unlike those of planetary nebulae.

   The UBV compilation (by Buscombe) apparently refers to BD+59.225, apparently
as a result of previous confusion.

GSC4030.149 011719.10 +602303.8 (2000.0)  9.07 1
GSC4030.149 011719.16 +602303.5 (2000.0)  9.01 1
USNO1500.01316161 011719.177 +602303.28 (2000.0)  8.0 10.7
IRAS01141+6007 011407.4 +600715 (1950.0)
    F12=0.76  F25=0.16  F60=0.40L F100=8.31L
    VAR=20 LRS=-1
 possibly I: oxygen-rich non-variable star without circumstellar shell
 or VIa: non-variable star with relatively cold dust at large
      distance, may be carbon-rich
011718.5 +602313 (2000.0) BD+59.224 9.3
011718.6 +602311 (2000.0) UBV_ 10.10 0.30 0.21 .007 .022 - B7 N=2 Nm=4 -
011718.7 +602303 (2000.0) MSX5C_G126.1261-02.3268 -29 -15 1 -2 -1 -4 V(%):-:-:2:-:-:-
011719.0 +602302 (2000.0) IRAS01141+6007 0.779 0.165 0.400L 8.235L 20%
011719.0 +602302 (2000.0) SSC01141+6007 0.779 0.165 0.400L 8.235L
011719.1 +602303 (2000.0) 950Vw 1.43 TYC4030.149.1 plx=-32.9(14.6) (0.02 0.04)
011719.0 +602302 (2000.0) 949 1.50 TYC2-4030.149.1 (9.65 0.02) (11.41 0.04)

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