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相关论文: WIYN Open Cluster Study. XXIV. Stellar Radial-Velo…

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We used high resolution spectra acquired at the Magellan Telescope to measure radial and rotational velocities of approximately 200 stars in the Galactic globular cluster NGC 3201. The surveyed sample includes Blue Stragglers Stars (BSSs)…

We present and analyse 120 spectroscopic binary and triple cluster members of the old (4 Gyr) open cluster M67 (NGC 2682). As a cornerstone of stellar astrophysics, M67 is a key cluster in the WIYN Open Cluster Study (WOCS); radial-velocity…

太阳与恒星天体物理 · 物理学 2021-03-24 Aaron M. Geller , Robert D. Mathieu , David W. Latham , Maxwell Pollack , Guillermo Torres , Emily M. Leiner

We present comprehensive cluster membership and g'r' photometry of the prototypical old, metal-rich Galactic star cluster NGC 6791. The proper-motion catalog contains 58,901 objects down to g'=24, limited to a circular area of radius 30…

太阳与恒星天体物理 · 物理学 2011-04-29 I. Platais , K. M. Cudworth , V. Kozhurina-Platais , D. E. McLaughlin , S. Meibom , C. Veillet

We have used a combination of high-resolution Hubble Space Telescope WFPC2 and wide-field ground-based observations, in ultraviolet and optical bands, to study the blue straggler star population of the massive outer-halo globular cluster…

星系天体物理 · 物理学 2013-11-07 N. Sanna , E. Dalessandro , F. R. Ferraro , B. Lanzoni , P. Miocchi , R. W. O'Connell

High-dispersion spectra of 89 potential members of the old, super-metal-rich open cluster, NGC 6253, have been obtained with the HYDRA multi-object spectrograph. Based upon radial-velocity measurements alone, 47 stars at the turnoff of the…

星系天体物理 · 物理学 2015-05-18 B. J. Anthony-Twarog , C. P. Deliyannis , B. A. Twarog , J. D. Cummings , R. M. Maderak

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…

NGC 6809 is a luminous metal-poor halo globular cluster that is relatively easy to study due to its proximity and low concentration. Because of its high Galactic latitude (b = -23deg), interstellar reddening and contamination is not very…

太阳与恒星天体物理 · 物理学 2015-06-05 Devesh P. Sariya , R. K. S. Yadav , A. Bellini

We present the list of variable stars we found in the Kepler superstamp data covering approximately 9 arcminutes from the central region of NGC 6791. We classified the variable stars based on the variability type and we established their…

太阳与恒星天体物理 · 物理学 2023-03-15 Sachu Sanjayan , Andrzej S Baran , Peter Nemeth , Karen Kinemuchi , Jakub Ostrowski , Sumanta Kumar Sahoo

NGC 6819 is a richly populated, older open cluster situated within the Kepler field. A CCD survey of the cluster on the uvbyCaHbeta system, coupled with proper-motion membership, has been used to isolate 382 highly probable, single-star…

太阳与恒星天体物理 · 物理学 2015-06-22 B. J. Anthony-Twarog , C. P. Deliyannis , B. A. Twarog

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 35 new spectroscopic-binary orbits from our extended radial-velocity (RV) survey of the old ($6.4 \pm 0.2$ Gyr) open cluster NGC 188. Using data from the WIYN Open Cluster Study (WOCS) and APOGEE-2, this work nearly doubles the…

太阳与恒星天体物理 · 物理学 2026-01-21 Ritvik Sai Narayan , Evan Linck , Robert D. Mathieu , Aaron M. Geller

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…

星系天体物理 · 物理学 2010-11-17 Warren J. Hankey , Andrew A. Cole

We present an updated catalog of stellar rotation periods for the 2.5 Gyr open cluster NGC 6819 using the Kepler IRIS light curves from superstamp data. Our analysis uses Gaussian Process modeling to extract robust rotation signals from…

太阳与恒星天体物理 · 物理学 2025-10-03 Sabina Sagynbayeva , Isabel L. Colman , Will M. Farr

The old and metal rich open cluster NGC 6253 was observed with the FLAMES multi-object spectrograph during an extensive radial velocity campaign monitoring 317 stars with a median of 15 epochs per object. All the targeted stars are located…

地球与行星天体物理 · 物理学 2016-02-17 M. Montalto , C. H. F. Melo , N. C. Santos , D. Queloz , G. Piotto , S. Desidera , L. R. Bedin , Y. Momany , I. Saviane

We measured the radial velocity of 139 stars in the region of NGC 6253, discussing cluster's membership and binarity in this sample, complementing our analysis with photometric, proper motion, and radial velocity data available from…

星系天体物理 · 物理学 2015-05-18 M. Montalto , S. Villanova , J. Koppenhoefer

We made a survey of the variable stars in a $13.2 \times 13.2$ arcmin$^2$ centered on the field of the Galactic bulge cluster NGC 6558. A total of 78 variables was found in the field of the cluster. Many of these variables are included in…

太阳与恒星天体物理 · 物理学 2024-07-02 A. Arellano Ferro , L. J. Zerpa Guillen , M. A. Yepez , I. H. Bustos Fierro , Z. Prudil , C. E. Pérez Parra

We present 236 new radial velocities of galaxies in the cluster A2256 measured with the WIYN Hydra multi-object spectrograph. Combined with the previous work of Fabricant, Kent, and Kurtz (1989), we have velocities for a total of 319…

天体物理学 · 物理学 2009-11-07 R. C. Berrington , P. M. Lugger , H. N. Cohn

We present stellar variability towards the young open cluster NGC\,6823. Time series $V$- and $I$-band CCD photometry led to identification and characterization of 88 variable stars, of which only 14 have been previously recognized. We…

We present a list of 72 radial velocity member stars in the metal-rich globular cluster NGC5927. The radial velocities are based on multi-epoch, multi-fibre spectra. We identify 46 RGB/HB stars and 26 turn-off stars that are radial velocity…

星系天体物理 · 物理学 2013-07-17 J. Simmerer , S. Feltzing , F. Primas

In an optical color-magnitude diagram sub-subgiants (SSGs) lie red of the main sequence and fainter than the base of the red giant branch in a region not easily populated by standard stellar-evolution pathways. In this paper, we present…

太阳与恒星天体物理 · 物理学 2016-06-01 Katelyn E. Milliman , Emily Leiner , Robert D. Mathieu , Benjamin M. Tofflemire , Imants Platais