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Query : 2000ApJ...538..289Z |
2000ApJ...538..289Z - Astrophys. J., 538, 289-294 (2000/July-3)
On the helium content of galactic globular clusters via the r-parameter.
ZOCCALI M., CASSISI S., BONO G., PIOTTO G., RICH R.M. and DJORGOVSKI S.G.
Abstract (from CDS):
The trend in the R-parameter toward solar metallicity is consistent with an upper limit to the He-to-metal enrichment ratio of the order of 2.5. Detailed calculations of central He burning times as a function of the horizontal-branch (HB) morphology suggest that He lifetimes for hot HB stars are on average ~20% longer than for RR Lyrae and red HB stars. Therefore, the increase in the empirical R-values of metal-poor clusters characterized by blue HB morphologies is due to an increase in the HB lifetime and not due to an increase in the He abundance.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: Globular Clusters: General - Stars: Abundances - Stars: Evolution - Stars: Horizontal-Branch
Simbad objects: 30
Number of rows : 30 |
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 | NGC 104 | GlC | 00 24 05.359 | -72 04 53.20 | 4.09 | ~ | 3914 | 0 | ||||
2 | NGC 362 | GlC | 01 03 14.26 | -70 50 55.6 | 6.58 | ~ | 1084 | 0 | ||||
3 | NGC 1851 | GlC | 05 14 06.76 | -40 02 47.6 | ~ | 1429 | 0 | |||||
4 | M 79 | GlC | 05 24 10.59 | -24 31 27.3 | 8.16 | ~ | 816 | 0 | ||||
5 | NGC 2808 | GlC | 09 12 03.10 | -64 51 48.6 | ~ | 1419 | 0 | |||||
6 | M 68 | GlC | 12 39 27.98 | -26 44 38.6 | 7.96 | ~ | 997 | 0 | ||||
7 | NGC 5634 | GlC | 14 29 37.28 | -05 58 35.1 | 10.69 | 10.05 | ~ | 300 | 0 | |||
8 | NGC 5694 | GlC | 14 39 36.52 | -26 32 18.0 | ~ | 301 | 0 | |||||
9 | NGC 5824 | GlC | 15 03 58.612 | -33 04 06.70 | 10.28 | 9.56 | ~ | 408 | 0 | |||
10 | NGC 5927 | GlC | 15 28 00.69 | -50 40 22.9 | ~ | 462 | 0 | |||||
11 | NGC 5946 | GlC | 15 35 28.58 | -50 39 35.0 | ~ | 194 | 0 | |||||
12 | M 80 | GlC | 16 17 02.41 | -22 58 33.9 | ~ | 715 | 0 | |||||
13 | NGC 6139 | GlC | 16 27 39.987 | -38 50 57.03 | 11.03 | 9.68 | ~ | 214 | 0 | |||
14 | M 13 | GlC | 16 41 41.634 | +36 27 40.75 | 5.8 | ~ | 2191 | 0 | ||||
15 | NGC 6235 | GlC | 16 53 25.36 | -22 10 38.8 | 11.99 | 7.20 | ~ | 186 | 0 | |||
16 | M 19 | GlC | 17 02 37.69 | -26 16 04.6 | 8.45 | 5.57 | ~ | 369 | 1 | |||
17 | NGC 6284 | GlC | 17 04 28.747 | -24 45 51.22 | 10.72 | 7.43 | ~ | 278 | 0 | |||
18 | NGC 6287 | GlC | 17 05 09.4906767360 | -22 42 28.099250172 | 11.49 | 10.30 | ~ | 224 | 0 | |||
19 | NGC 6293 | GlC | 17 10 10.42 | -26 34 54.2 | ~ | 281 | 0 | |||||
20 | NGC 6342 | GlC | 17 21 10.14 | -19 35 14.7 | 10.01 | ~ | 286 | 0 | ||||
21 | NGC 6356 | GlC | 17 23 34.99 | -17 48 46.9 | 10.01 | 7.42 | ~ | 350 | 1 | |||
22 | NGC 6362 | GlC | 17 31 54.99 | -67 02 54.0 | ~ | 585 | 0 | |||||
23 | NGC 6388 | GlC | 17 36 17.461 | -44 44 08.34 | ~ | 913 | 1 | |||||
24 | NGC 6441 | GlC | 17 50 13.06 | -37 03 05.2 | ~ | 884 | 0 | |||||
25 | NGC 6522 | GlC | 18 03 34.08 | -30 02 02.3 | ~ | 524 | 0 | |||||
26 | NGC 6624 | GlC | 18 23 40.51 | -30 21 39.7 | ~ | 885 | 1 | |||||
27 | NGC 6652 | GlC | 18 35 45.63 | -32 59 26.6 | ~ | 437 | 0 | |||||
28 | NGC 6934 | GlC | 20 34 11.37 | +07 24 16.1 | ~ | 422 | 0 | |||||
29 | M 72 | GlC | 20 53 27.70 | -12 32 14.3 | 8.96 | ~ | 430 | 0 | ||||
30 | M 15 | GlC | 21 29 58.33 | +12 10 01.2 | ~ | 3138 | 0 |
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