C-M diagram and luminosity function of the Galactic globular cluster NGC 7099. I - Photographic photometry

1987 ◽  
Vol 94 ◽  
pp. 360 ◽  
Author(s):  
Giampaolo Piotto ◽  
Massimo Capaccioli ◽  
Sergio Ortolani ◽  
Leonida Rosino ◽  
Gonzalo Alcaino ◽  
...  
Keyword(s):  
Globular Cluster ◽  
Luminosity Function ◽  
Photographic Photometry

scholarly journals The deep luminosity function of the globular cluster M30

1990 ◽  
Vol 350 ◽  
pp. 662 ◽  
Author(s):  
Giampaolo Piotto ◽  
Ivan R. King ◽  
Massimo Capaccioli ◽  
Sergio Ortolani ◽  
S. Djorgovski
Keyword(s):  
Globular Cluster ◽  
Luminosity Function

scholarly journals The HST large programme on NGC 6752 – III. Detection of the peak of the white dwarf luminosity function

2019 ◽  
Vol 488 (3) ◽  
pp. 3857-3865
Author(s):  
L R Bedin ◽  
M Salaris ◽  
J Anderson ◽  
M Libralato ◽  
D Apai ◽  
...  
Keyword(s):  
Globular Cluster ◽  
White Dwarf ◽  
Luminosity Function ◽  
Main Sequence ◽  
Hubble Space Telescope ◽  
Horizontal Branch ◽  
Space Telescope

ABSTRACT We report on the white dwarf (WD) cooling sequence of the old globular cluster NGC 6752, which is chemically complex and hosts a blue horizontal branch. This is one of the last globular cluster WD cooling sequences accessible to imaging by the Hubble Space Telescope. Our photometry and completeness tests show that we have reached the peak of the luminosity function of the WD cooling sequence, at a magnitude mF606W  = 29.4 ± 0.1, which is consistent with a formal age of ∼14 Gyr. This age is also consistent with the age from fits to the main-sequence turn-off (13–14 Gyr), reinforcing our conclusion that we observe the expected accumulation of WDs along the cooling sequence.

scholarly journals New Insights from a Study of the Globular Cluster Systems of 60 Early-Type Galaxies

2002 ◽  
Vol 207 ◽  
pp. 229-237
Author(s):  
Arunav Kundu ◽  
Brad Whitmore
Keyword(s):  
Globular Cluster ◽  
Surface Brightness ◽  
Luminosity Function ◽  
Photometric Study ◽  
Early Type ◽  
Color Distribution ◽  
Cluster Systems ◽  
Brightness Fluctuation ◽  
Distance Indicator ◽  
Fluctuation Method

We present the results of our detailed WFPC2-based photometric study of the globular cluster systems (GCS) of over 60 elliptical and SO galaxies. Approximately 50% of the GCSs of ellipticals, and at least 15–20% of S0s reveal bimodality in the color distribution. We trace the variation in GCS properties with Hubble type and discuss the implications on the various models of galaxy (and cluster system) formation. We also provide evidence that the globular cluster luminosity function is an excellent distance indicator with an accuracy comparable to the surface brightness fluctuation method.

scholarly journals Deep Wide-Field Photometry of the NGC 5128 Globular Cluster System: A Progress Report

2002 ◽  
Vol 207 ◽  
pp. 309-311
Author(s):  
G. L. H. Harris ◽  
D. Geisler ◽  
W. E. Harris ◽  
J. E. Hesser
Keyword(s):  
Globular Cluster ◽  
Luminosity Function ◽  
Progress Report ◽  
Cluster System ◽  
Wide Field ◽  
Preliminary Results ◽  
System A ◽  
Globular Cluster System

We have obtained CMR photometry for a roughly 1° square region centered on NGC 5128. Preliminary results indicate that the limiting magnitude of the images is ≳ 1 magnitude fainter than the peak of the globular cluster luminosity function (GCLF) at R ⋍ 21.

scholarly journals Trends in the Globular Cluster Luminosity Function of Early-Type Galaxies

2006 ◽  
Vol 651 (1) ◽  
pp. L25-L28 ◽  
Author(s):  
Andrés Jordán ◽  
Dean E. McLaughlin ◽  
Patrick Côté ◽  
Laura Ferrarese ◽  
Eric W. Peng ◽  
...  
Keyword(s):  
Globular Cluster ◽  
Luminosity Function ◽  
Early Type

Two-color photographic photometry of variables in the globular cluster M28

1990 ◽  
Vol 100 ◽  
pp. 686 ◽  
Author(s):  
Amelia Wehlau ◽  
Steven Butterworth
Keyword(s):  
Globular Cluster ◽  
Photographic Photometry

The Luminosity Function for the Globular Cluster M13

1968 ◽  
Vol 151 ◽  
pp. 133 ◽  
Author(s):  
Mahiro Simoda ◽  
Hiroshi Kimura
Keyword(s):  
Globular Cluster ◽  
Luminosity Function
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