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| Query : 2012PASP..124..922D |
2012PASP..124..922D - Publ. Astron. Soc. Pac., 124, 922-933 (2012)
MRI: A possible mechanism for funnel flows?
DOGAN S. and PEKUNLU E.R.
Journal keyword(s):
Simbad objects: 5
| Number of rows : 5 |
| 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 | NAME Andromeda II | G | 01 16 29.8 | +33 25 09 | 11.7 | ~ | 402 | 0 | ||||
| 2 | V* BP Tau | Or* | 04 19 15.8339827632 | +29 06 26.926959492 | 13.13 | 12.12 | 11.89 | K5/7Ve | 721 | 0 | ||
| 3 | V* TW Hya | TT* | 11 01 51.9053285064 | -34 42 17.033218380 | 11.94 | 10.50 | 10.626 | 9.18 | K6Ve | 2144 | 1 | |
| 4 | V* MN Lup | TT* | 15 23 30.3994838448 | -38 21 28.841024628 | 14.15 | M0 | 27 | 0 | ||||
| 5 | V* RU Lup | TT* | 15 56 42.3108692112 | -37 49 15.473946900 | 9.27 | 10.07 | 9.60 | K7/M0e | 528 | 0 |
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