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| Query : 2006MNRAS.372.1675S |
2006MNRAS.372.1675S - Mon. Not. R. Astron. Soc., 372, 1675-1680 (2006/November-2)
The RR Lyrae period-K-luminosity relation for globular clusters: an observational approach.
SOLLIMA A., CACCIARI C. and VALENTI E.
Abstract (from CDS):
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): methods: observational - techniques: photometric - stars: distances - stars: variables: other - infrared: stars
Simbad objects: 18
| Number of rows : 18 |
| 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 | M 31 | AGN | 00 42 44.330 | +41 16 07.50 | 4.86 | 4.36 | 3.44 | ~ | 13622 | 1 | ||
| 2 | NAME Ret | GlC | 04 36 10.15 | -58 51 34.8 | 14.00 | 14.25 | 13.50 | ~ | 177 | 1 | ||
| 3 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 19090 | 0 | ||||
| 4 | NGC 3201 | GlC | 10 17 36.82 | -46 24 44.9 | ~ | 1001 | 0 | |||||
| 5 | M 68 | GlC | 12 39 27.98 | -26 44 38.6 | 7.96 | ~ | 1069 | 0 | ||||
| 6 | NGC 5139 | GlC | 13 26 47.28 | -47 28 46.1 | ~ | 3677 | 0 | |||||
| 7 | M 3 | GlC | 13 42 11.62 | +28 22 38.2 | 6.39 | ~ | 2593 | 0 | ||||
| 8 | IC 4499 | GlC | 15 00 18.57 | -82 12 49.6 | 8.56 | ~ | 375 | 0 | ||||
| 9 | NGC 5897 | GlC | 15 17 24.40 | -21 00 36.4 | 10.16 | 8.52 | ~ | 424 | 0 | |||
| 10 | M 5 | GlC | 15 18 33.22 | +02 04 51.7 | 5.95 | ~ | 2095 | 0 | ||||
| 11 | M 4 | GlC | 16 23 35.22 | -26 31 32.7 | ~ | 1978 | 0 | |||||
| 12 | M 107 | GlC | 16 32 31.86 | -13 03 13.6 | ~ | 835 | 0 | |||||
| 13 | M 92 | GlC | 17 17 07.39 | +43 08 09.4 | 6.52 | ~ | 2240 | 0 | ||||
| 14 | NGC 6362 | GlC | 17 31 54.99 | -67 02 54.0 | ~ | 637 | 0 | |||||
| 15 | NGC 6584 | GlC | 18 18 37.60 | -52 12 56.8 | 8.17 | ~ | 317 | 0 | ||||
| 16 | M 22 | GlC | 18 36 23.94 | -23 54 17.1 | ~ | 1459 | 0 | |||||
| 17 | M 55 | GlC | 19 39 59.71 | -30 57 53.1 | 6.49 | ~ | 913 | 0 | ||||
| 18 | M 15 | GlC | 21 29 58.33 | +12 10 01.2 | ~ | 3274 | 0 |
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