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相关论文: The Rotation of Sub-Populations in omega Centauri

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We present results of an extensive spectroscopic survey of Subgiant stars in the stellar system omega Centauri. Using infrared CaII triplet lines, we derived metallicities and radial velocities for more than 250 stars belonging to different…

天体物理学 · 物理学 2009-11-13 A. Sollima , E. Pancino , F. R. Ferraro , M. Bellazzini , O. Straniero , L. Pasquini

I present some preliminary results from a high-resolution spectroscopic observing campaign conducted with UVES at the ESO VLT, devoted to the study of the newly discovered, metal-rich red giant branch (RGB-a) in omega Centauri. In…

天体物理学 · 物理学 2007-05-23 E. Pancino

We present wide-field and high-precision BV and Ca & Stromgren by photometry of omega Centauri, which represents one of the most extensive photometric surveys to date for this cluster. The member stars of omega Cen are well discriminated…

天体物理学 · 物理学 2009-11-10 S. -C. Rey , Y. -W. Lee , C. Ree , J. -M. Joo , Y. -J. Sohn , A. Walker

Our recent CCD photometry (Lee et al. 1999) has shown, for the first time, that omega Cen has several distinct stellar populations, which is reminiscent of the Sagittarius dwarf galaxy. Here we present more detailed analysis of the data…

We present a near-infrared J and K photometric catalog containing more than 73,000 stars in the central region of the giant Globular Cluster omega Centauri. This is the largest IR data-set ever published for this cluster and has been used…

天体物理学 · 物理学 2009-11-10 A. Sollima , F. R. Ferraro , L. Origlia , E. Pancino , M. Bellazzini

Using deep high-resolution multi-band images taken with the Very Large Telescope and the Hubble Space Telescope, we discovered a new anomalous sequence in the Color Magnitude Diagram of omega Cen. This feature appears as a narrow,…

天体物理学 · 物理学 2009-11-10 F. R. Ferraro , A. Sollima , E. Pancino , M. Bellazzini , O. Straniero , L. Origlia , A. M. Cool

We report the results of an extensive VLT high-resolution imaging campaign of the central region of the giant globular cluster omega Centauri. More than 100,000 stars have been measured in the inner 9'x 9' region of the cluster. On the…

天体物理学 · 物理学 2011-07-18 A. Sollima , F. R. Ferraro , E. Pancino , M. Bellazzini

We report on the complex structure of the red giant branch (RGB) of omega Cen, based on a new wide field and wide color baseline B and I photometry. Our color magnitude diagram (CMD) shows the presence of multiple populations along this…

天体物理学 · 物理学 2009-10-05 E. Pancino , F. R. Ferraro , M. Bellazzini , G. Piotto , M. Zoccali

Near-infrared spectra of 21 giants in omega Centauri, spanning the whole range of metallicities observed in this cluster, are presented. This work is part of a coordinated photometric and spectroscopic campaign in the optical and in the…

天体物理学 · 物理学 2009-11-07 L. Origlia , F. R. Ferraro , M. Bellazzini , E. Pancino

I present preliminary results for a sample of ~700 red giants in omega Cen, observed during the Ital-FLAMES Consortium GTO time in May 2003, for the Bologna Project on omega Cen. Preliminary Fe and Ca abundances confirm previous results:…

天体物理学 · 物理学 2015-06-24 E. Pancino

We analyze spectra of 18 stars belonging to the faintest subgiant branch in omega Centauri (the SGB-a), obtained with GIRAFFE@VLT at a resolution o R~17000 and a S/N ratio between 25 and 50. We measure abundances of Al, Ba, Ca, Fe, Ni, Si,…

星系天体物理 · 物理学 2015-05-30 E. Pancino , A. Mucciarelli , P. Bonifacio , L. Monaco , L. Sbordone

We present a detailed study of the radial distribution of the multiple populations identified in the Galactic globular cluster omega Cen. We used both space-based images (ACS/WFC and WFPC2) and ground-based images (FORS1@VLT and [email protected]

太阳与恒星天体物理 · 物理学 2014-11-20 A. Bellini , G. Piotto , L. R. Bedin , I. R. King , J. Anderson , A. P. Milone , Y. Momany , .

We present radial velocities, Fe, and Al abundances for 180 red giant branch (RGB) stars in the Galactic globular cluster Omega Centauri ($\omega$ Cen). The majority of our data lie in the range 11.0$<$V$<$13.5, which covers the RGB from…

天体物理学 · 物理学 2009-11-13 Christian I. Johnson , Catherine A. Pilachowski , Jennifer Simmerer , Dustin Schwenk

We analysed high-resolution UVES spectra of six stars belonging to the subgiant branch of omega Centauri, and derived abundance ratios of 19 chemical elements (namely Al, Ba, C, Ca, Co, Cr, Cu, Fe, La, Mg, Mn, N, Na, Ni, Sc, Si, Sr, Ti, and…

太阳与恒星天体物理 · 物理学 2015-05-20 E. Pancino , A. Mucciarelli , L. Sbordone , M. Bellazzini , L. Pasquini , L. Monaco , F. R. Ferraro

We present spectroscopic abundances and radial velocities for giant stars in the Galactic globular cluster omega Centauri based on the CaII infrared triplet. Two samples of stars were observed: 234 stars at M_V = 1.25 on the lower giant…

天体物理学 · 物理学 2009-10-05 Nicholas B. Suntzeff , Robert P. Kraft

We present multi-wavelength observations of the northern population of Omega Cen from the main-sequence turn-off to high on the red giant branch. We show that the best information about the metallicity and age of the stars can be gained…

天体物理学 · 物理学 2016-08-30 Joanne Hughes , George Wallerstein , Floor van Leeuwen

A revised metallicity calibration of the Stroemgren (b-y),m_1 diagram, based on a sample of globular cluster and field red giant stars, is presented. This new calibration has been used to determine Stroemgren metallicities ([Fe/H]_phot) for…

天体物理学 · 物理学 2007-05-23 M. Hilker , T. Richtler

We present new intermediate-band Stroemgren photometry based on more than 300 u,v,b,y images of the Galactic globular cluster Omega Cen. Optical data were supplemented with new multiband near-infrared (NIR) photometry (350 J,H,K_s images).…

We present wide-field and high-precision BV and Ca & Stromgren by photometry of omega Centauri and its RR Lyrae stars, which represents one of the most extensive photometric surveys to date for this cluster. The member stars of omega Cen…

天体物理学 · 物理学 2007-05-23 Soo-Chang Rey , Jong-Myung Joo , Young-Jong Sohn , Chang H. Ree , Young-Wook Lee , Alistair Walker

We present a metallicity distribution based on photometry and spectra for 442 omega Cen cluster members that lie at the main sequence turnoff region of the color-magnitude diagram. This distribution is similar to that found for the red…

天体物理学 · 物理学 2011-02-11 L. M. Stanford , G. S. Da Costa , J. E. Norris , R. D. Cannon
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