Results 41 to 50 of about 7,252,313 (352)

UKIRT follow-up observations of the old open cluster FSR0358 (Kirkpatrick1) [PDF]

open access: yes, 2009
We aim to characterise the properties of the stellar clusters in the Milky Way. Utilising an expectation-maximisation method we determined that the cluster FSR0358, originally discovered by J.D.Kirkpatrick, is the most likely real cluster amongst the ...
Bertin   +29 more
core   +2 more sources

WIYN Open Cluster Study 89. M48 (NGC 2548) 2: Lithium Abundances in the 420 Myr Open Cluster M48 from Giants through K Dwarfs

open access: yesThe Astrophysical Journal, 2023
We consider WIYN/Hydra spectra of 329 photometric candidate members of the 420 Myr old open cluster M48 and report lithium detections or upper limits for 234 members and likely members.
Qinghui Sun   +4 more
doaj   +1 more source

The highly polarized open cluster Trumpler 27 [PDF]

open access: yes, 2000
We have carried out multicolor linear polarimetry (UBVRI) of the brightest stars in the area of the open cluster Trumpler 27. Our data show a high level of polarization in the stellar light with a considerable dispersion, from $P = 4%$ to $P = 9.5%$. The
Axon D. J.   +12 more
core   +3 more sources

A Machine-learning-based Investigation of the Open Cluster M67

open access: yesAstrophysical Journal, 2018
In this paper, we use a machine-learning method, random forest (RF), to identify reliable members of the old (4 Gyr) open cluster M67 based on the high-precision astrometry and photometry taken from the second Gaia data release (Gaia-DR2).
Xinhua Gao
semanticscholar   +1 more source

Characterization of open cluster remnants

open access: yes, 2007
Despite progress in the theoretical knowledge of open cluster remnants and the growing search for observational identifications in recent years, open questions still remain. The methods used to analyze open cluster remnants and criteria to define them as
Bica, E., Pavani, D. B
core   +1 more source

STELLAR RADIAL VELOCITIES IN THE OLD OPEN CLUSTER M67 (NGC 2682). I. MEMBERSHIPS, BINARIES, AND KINEMATICS [PDF]

open access: yes, 2015
We present results from 13776 radial-velocity (RV) measurements of 1278 candidate members of the old (4 Gyr) open cluster M67 (NGC 2682). The measurements are the results of a long-term survey that includes data from seven telescopes with observations ...
A. Geller, D. Latham, R. Mathieu
semanticscholar   +1 more source

SS Lac in Open Cluster NGC 7209 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 1997
We present IUE observations in far ultraviolet region for SS Lac in open cluster NGC 7209. The IUE short wavelength spectrum and long wavelength spectrum were merged to produce an energy distribution curve between 1200A and 3200A.
Young Woon Kang
doaj  

WIYN OPEN CLUSTER STUDY. XXXII. STELLAR RADIAL VELOCITIES IN THE OLD OPEN CLUSTER NGC 188 [PDF]

open access: yes, 2015
We present the results of our ongoing radial-velocity (RV) survey of the old (7 Gyr) open cluster NGC 188. Our WIYN 3.5 m data set spans a time baseline of 11 years, a magnitude range of 12 ⩽ V ⩽ 16.5 (1.18–0.94 M☉), and a 1° diameter region on the sky ...
A. Geller   +3 more
semanticscholar   +1 more source

Astrometric and photometric study of the open cluster NGC 2323 [PDF]

open access: yesSerbian Astronomical Journal, 2017
We present a study of the open cluster NGC 2323 using astrometric and photometric data. In our study we used two methods that are able to separate open cluster’s stars from those that belong to the stellar background. Our results of calculations
Amin M.Y., Elsanhoury W.H.
doaj   +1 more source

A statistical method to determine open cluster metallicities [PDF]

open access: yes, 2010
The study of open cluster metallicities helps to understand the local stellar formation and evolution throughout the Milky Way. Its metallicity gradient is an important tracer for the Galactic formation in a global sense.
Andrievsky   +56 more
core   +1 more source

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