Table 1
List of spectroscopically confirmed carbon stars and their photometric characteristics.
N° | DFBS Ident. | Sp. Type | V | B | R | B − R | J | H | Ks | J − Ks | Var. | Notes |
mag | mag | mag | mag | mag | mag | mag | mag | |||||
|
||||||||||||
1 | J003700.13+342234.0 | CH | 12.29 | 14.22 | 11.27 | 2.95 | 9.484 | 8.663 | 8.438 | 1.046 | ||
2 | J004619.15+354537.3 | CH | 13.61 | 15.20 | 13.00 | 2.20 | 11.795 | 11.252 | 11.115 | 0.680 | ||
3 | J020008.95+413747.4 | N | 14.93 | 16.76 | 14.27 | 2.50 | 10.867 | 9.549 | 8.656 | 2.211 | Semi Reg. | (1) |
4 | J032912.92+445330.0 | N | 15.06 | 19.20 | 13.50 | 5.70 | 9.157 | 7.838 | 6.875 | 2.282 | (2) | |
5 | J064958.54+741610.1 | N | 15.62 | 18.59 | 12.42 | 6.17 | 9.141 | 7.526 | 6.159 | 2.982 | Mira | (3) |
6 | J115153.56+412232.9 | CH | 13.25 | 14.65 | 12.57 | 2.08 | 11.601 | 11.056 | 10.959 | 0.632 | ||
7 | J135831.62+671042.7 | CH | 13.62 | 15.22 | 12.93 | 2.29 | 11.213 | 10.514 | 10.320 | 0.893 | ||
8 | J145241.15+785923.8 | CH | 13.51 | 15.65 | 13.08 | 2.57 | 10.985 | 10.237 | 9.976 | 1.009 | dC? | |
9 | J172734.59+651110.4 | CH | 12.32 | 13.72 | 11.78 | 1.94 | 9.922 | 9.195 | 8.982 | 0.940 | ||
10 | J172825.82+700829.6 | N | 13.78 | 17.91 | 14.14 | 3.77 | 11.537 | 10.117 | 9.022 | 2.515 | (4) | |
11 | J190034.62+440829.1 | CH | 12.10 | 13.15 | 11.06 | 2.09 | 9.951 | 9.373 | 9.146 | 0.805 | dC? | |
12 | J230835.19+403533.9 | N | 14.35 | 16.36 | 13.42 | 2.96 | 10.445 | 8.924 | 7.799 | 2.646 | Mira | (5) |
13 | J234043.43+353104.4 | CH | 14.24 | 16.11 | 13.36 | 2.75 | 11.429 | 10.685 | 10.397 | 1.032 | dC? |
Notes. The DFBS identification (Col. 2) is coded as JHHMMSS.ss+DDMMSS.s. – (1) and (5): these stars (identified with 2MASS J02000890+4137474 and 2MASS J23083509+4035344 respectively) are rediscovered (Neill Reid et al. 2008). – (2): Identified with IRAS 03257+4443 – (3): Erroneously classified as M8-M9 subtype star in the VI list of the FBS Late-Type Stars (Abrahamian & Gigoyan 1995). Identified with IRAS 06435+7419 – (4): Mauron et al. (2004). Identified with IRAS 17289+7010.
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