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Related papers: The Global Kinematics of the Globular Cluster M92

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We present velocities for 230 stars in the outer parts of the globular cluster M15 measured with the Hydra multi-object spectrograph on the WIYN telescope. A new Bayesian technique is used for analyzing the data. The mean velocity of the…

We present the measurement of radial velocities for globular clusters in M60, giant elliptical galaxy in the Virgo cluster. Target globular cluster candidates were selected using the Washington photometry based on the deep $16\arcmin \times…

We use Gaia Data Release 2 to determine the mean proper motions for 150 Milky Way globular clusters (almost the entire known population), with a typical uncertainty of 0.05 mas/yr limited mainly by systematic errors. Combining them with…

Astrophysics of Galaxies · Physics 2019-01-23 Eugene Vasiliev

Radial velocities are presented for a new sample of globular clusters in the outer halo of M87 at a distance of 300 to 540 arcsec (24 to 43 kpc) from the center of this galaxy. These are used to augment our previously published data and an…

Astrophysics · Physics 2009-10-31 Judith G. Cohen

B,V CCD frames have been used to derive surface brightness profiles for NGC 3201 out to ~18 arcmin. A total of 857 radial velocities with median precision ~1 km/s for 399 member giants have been used to trace the velocity dispersion profile…

Astrophysics · Physics 2009-10-28 Patrick Cote , Douglas L. Welch , Philippe Fischer , K. Gebhardt

We present the results from a study of the dynamics of the system of globular clusters around M87. After eliminating foreground galactic stars and background galaxies, we end up with a sample of 205 bona fide M87 globular clusters for which…

Astrophysics · Physics 2009-10-30 Judith G. Cohen , Anton Ryzhov

We have analyzed high dispersion and high precision spectra of 5 blue horizontal branch stars in the globular cluster M92 to establish that the projected rotational velocity for these stars ranges from 15 to 40 \kms. This is larger than…

Astrophysics · Physics 2009-10-30 J. G. Cohen , J. K. McCarthy

We present a detailed study of the internal kinematics of the Galactic Globular Cluster M 4 (NGC 6121), by deriving the radial velocities from 7250 spectra for 2771 stars distributed from the upper part of the Red Giant Branch down to the…

Astrophysics of Galaxies · Physics 2015-10-21 L. Malavolta , G. Piotto , L. R. Bedin , C. Sneden , V. Nascimbeni , V. Sommariva

We study the kinematics and dynamics of the globular cluster system of NGC 1399, the central galaxy of the Fornax cluster. The observational data consists of medium resolution spectra, obtained at the Very Large Telescope. Our sample…

We present 5201 radial-velocity measurements of 1144 stars, as part of an ongoing study of the young (150 Myr) open cluster M35 (NGC 2168). We have observed M35 since 1997, using the Hydra Multi-Object Spectrograph on the WIYN 3.5m…

Solar and Stellar Astrophysics · Physics 2015-05-14 Aaron M. Geller , Robert D. Mathieu , Ella K. Braden , Soren Meibom , Imants Platais , Christopher J. Dolan

We present new number density and surface brightness profiles for the globular cluster M92 (NGC 6341). These profiles are calculated from optical images collected with the CCD mosaic camera MegaCam at the Canada-France-Hawaii-Telescope and…

Solar and Stellar Astrophysics · Physics 2015-06-12 A. Di Cecco , A. Zocchi , A. L. Varri , M. Monelli , G. Bertin , G. Bono , P. B. Stetson , M. Nonino , R. Buonanno , I. Ferraro , G. Iannicola , A. Kunder , A. R. Walker

We have used the ARGUS multi-object spectrometer at the CTIO 4m Blanco telescope to obtain 2756 radial velocity measurements for 1966 individual stars in the globular cluster omega Centauri brighter than blue photographic magnitude of about…

We report on the radial velocity measurements of 18 globular clusters and one dE galaxy in the field of the giant elliptical galaxy NGC 1399, the dominant galaxy of the Fornax cluster. We present also the radial velocity measurements of…

Astrophysics · Physics 2009-10-30 Dante Minniti , Markus Kissler-Patig , Paul Goudfrooij , Georges Meylan

We present radial velocity and metallicity measurements for the far-southern Galactic globular cluster IC4499. We selected several hundred target red giant stars in and around the cluster from the 2MASS point source catalog, and obtained…

Astrophysics of Galaxies · Physics 2010-11-17 Warren J. Hankey , Andrew A. Cole

We have determined masses, stellar mass functions and structural parameters of 112 Milky Way globular clusters by fitting a large set of N-body simulations to their velocity dispersion and surface density profiles. The velocity dispersion…

Astrophysics of Galaxies · Physics 2018-07-03 H. Baumgardt , M. Hilker

Using the recently commissioned multi-object spectrograph AAOmega on the 3.9m AAT we have obtained medium-resolution near-infrared spectra for 10,500 stars in and around five southern globular clusters. The targets were 47 Tuc, M12, M30,…

Astrophysics · Physics 2009-11-13 P. Székely , L. L. Kiss , K. Szatmáry , B. Csák , G. Á. Bakos , T. R. Bedding

We present the results of a study aimed at characterizing the kinematics of the inner regions of the halo globular cluster M75 (NGC 6864) based on data acquired as part of the ESO-VLT Multi-Instrument Kinematic Survey (MIKiS) of Galactic…

We present a detailed kinematic analysis of the outer halo globular cluster (GC) system of M31. Our basis for this is a set of new spectroscopic observations for 78 clusters lying at projected distances between Rproj ~20-140 kpc from the…

A test of Newton's law of gravity in the low acceleration regime using globular clusters is presented. New results for the core collapsed globular cluster NGC 7099 are given. The run of the gravitational potential as a function of distance…

Astrophysics · Physics 2009-11-11 Riccardo Scarpa , Gianni Marconi , Roberto Gilmozzi , Giovanni Carraro

We present radial velocities for 85 cool stars projected onto the central parsec of the Galaxy. The majority of these velocities have relative errors of $\sim$1 km/s, or a factor of $\sim$30-100 smaller than those previously obtained with…

Astrophysics · Physics 2009-11-10 Donald F. Figer
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