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Query : 2014MNRAS.445L..94D |
2014MNRAS.445L..94D - Mon. Not. R. Astron. Soc., 445, L94-L98 (2014/November-3)
Why should we correct reported pulsation frequencies for stellar line-of-sight Doppler velocity shifts?
DAVIES G.R., HANDBERG R., MIGLIO A., CAMPANTE T.L., CHAPLIN W.J. and ELSWORTH Y.
Abstract (from CDS):
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): methods: data analysis - stars: oscillations
Simbad objects: 11
Number of rows : 11 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | V* ZZ Cet | WD* | 01 36 13.6153974672 | -11 20 32.632874601 | 14.328 | 14.16 | 14.4 | DA4.0 | 291 | 0 | ||
2 | HD 52265 | PM* | 07 00 18.0357115416 | -05 22 01.780929120 | 6.845 | 6.282 | G0V | 329 | 1 | |||
3 | HD 169392A | SB* | 18 24 42.9854204880 | -06 36 13.674463524 | 7.98 | 7.41 | G0IV | 41 | 0 | |||
4 | HD 173701 | PM* | 18 44 35.1191008536 | +43 49 59.790008892 | 8.37 | 7.52 | G8V | 178 | 0 | |||
5 | BD+42 3187 | RG* | 18 54 16.9544655840 | +42 59 00.384912816 | 10.495 | 9.939 | 10.086 | G2 | 85 | 0 | ||
6 | BD+41 3306 | PM* | 19 19 00.5489000285 | +41 38 04.582441681 | 10.01 | 9.67 | 8.86 | 8.18 | 7.66 | K0V | 287 | 0 |
7 | V* RR Lyr | RR* | 19 25 27.9129605304 | +42 47 03.693258204 | 7.36 | 7.6 | kA3hF0 | 926 | 0 | |||
8 | Kepler-56 | RG* | 19 35 02.0011980936 | +41 52 18.692360400 | 13.954 | 12.756 | 12.379 | ~ | 174 | 1 | ||
9 | * 16 Cyg A | ** | 19 41 48.9534996168 | +50 31 30.219536784 | 6.79 | 6.59 | 5.95 | 5.50 | 5.17 | G1.5Vb | 762 | 0 |
10 | * 16 Cyg | ** | 19 41 49.09 | +50 31 31.6 | ~ | 152 | 0 | |||||
11 | * 16 Cyg B | PM* | 19 41 51.9726777456 | +50 31 03.089030916 | 7.07 | 6.86 | 6.20 | 5.76 | 5.42 | G3V | 890 | 1 |
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