1999ApJ...522..983F


Query : 1999ApJ...522..983F

1999ApJ...522..983F - Astrophys. J., 522, 983-990 (1999/September-2)

Blue straggler stars: the spectacular population in M80.

FERRARO F.R., PALTRINIERI B., ROOD R.T. and DORMAN B.

Abstract (from CDS):

Using Hubble Space Telescope WFPC2 observations in two ultraviolet (UV) filters (F225W and F336W) of the central region of the high-density Galactic globular cluster (GGC) M80, we have identified 305 blue straggler stars (BSS), which represents the largest and most concentrated population of BSS ever observed in a GGC. We also identify the largest clean sample of evolved BSS yet found. The high stellar density alone cannot explain the BSS, and we suggest that in M80 we are witnessing a transient dynamical state, during which stellar interactions are delaying the core-collapse process leading to an exceptionally large population of collisional BSS.

Abstract Copyright:

Journal keyword(s): Stars: Blue Stragglers - Galaxy: Globular Clusters: Individual: Messier Number: M80 - Stars: Evolution - Ultraviolet: Stars

Nomenclature: Table 1, col(1): Cl* NGC 6093 BSS NNN (Nos 1-305) = Table 1, col(2): Cl* NGC 6093 FPR NNNNN N=305 among 13000. Table 2, col(1): Cl* NGC 6093 EBSS NN (Nos 1-19) = Table 2, col(2): Cl* NGC 6093 FPR NNNNN N=19 among 13000.

Status at CDS : Large table(s) of objects being ingested in VizieR. // All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 8

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Number of rows : 8
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     ~ 3917 0
2 NGC 2808 GlC 09 12 03.10 -64 51 48.6           ~ 1420 0
3 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2479 0
4 M 80 GlC 16 17 02.41 -22 58 33.9           ~ 716 0
5 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2193 0
6 M 92 GlC 17 17 07.39 +43 08 09.4     6.52     ~ 2116 0
7 NGC 6388 GlC 17 36 17.461 -44 44 08.34           ~ 914 1
8 M 30 GlC 21 40 22.12 -23 10 47.5     7.10     ~ 1049 0

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