中文
相关论文

相关论文: Hubble Space Telescope Observations of an Outer Fi…

200 篇论文

Recent, high precision photometry of Omega Centauri, the biggest Galactic globular cluster, has been obtained with Hubble Space Telescope. The color magnitude diagram reveals an unexpected bifurcation of colors in the main sequence (MS).…

天体物理学 · 物理学 2007-05-23 L. R. Bedin , G. Piotto , J. Anderson , I. R. King , S. Cassisi , Y. Momany , .

Recent observations for the color-magnitude diagrams (CMDs) of the massive globular cluster Omega Centauri have shown that it has a striking double main sequence (MS), with a minority population of bluer and fainter MS well separated from a…

The globular cluster omega Centauri contains the largest known population of very hot horizontal branch (HB) stars. We have used the Hubble Space Telescope to obtain a far-UV/optical color-magnitude diagram of three fields in omega Cen. We…

As part of a large investigation with Hubble Space Telescope to study the faintest stars within the globular cluster Omega Centauri, in this work we present early results on the multiplicity of its main sequence (MS) stars, based on deep…

太阳与恒星天体物理 · 物理学 2017-05-31 A. P. Milone , A. F. Marino , L. R. Bedin , J. Anderson , D. Apai , A. Bellini , P. Bergeron , A. J. Burgasser , A. Dotter , J. M. Rees

High spectral resolution and high signal-to-noise ratio optical spectra of red giants in the globular cluster Omega Centauri are analysed for stellar parameters and chemical abundances of 15 elements including helium by either line…

太阳与恒星天体物理 · 物理学 2020-05-20 Arumalla B. S. Reddy

The globular cluster $\omega$ Centauri (NGC 5139) is a puzzling stellar system harboring several distinct stellar populations whose origin still represents a unique astrophysical challenge. Current scenarios range from primordial chemical…

星系天体物理 · 物理学 2014-11-20 Sandro Villanova , Giovanni Carraro , Riccardo Scarpa , Gianni Marconi

In the fourth paper of this series, we present -- and publicly release -- the state-of-the-art catalogue and atlases for the two remaining parallel fields observed with the Hubble Space Telescope for the large programme on omega Centauri.…

太阳与恒星天体物理 · 物理学 2021-07-20 M. Scalco , A. Bellini , L. R. Bedin , J. Anderson , P. Rosati , M. Libralato , M. Salaris , E. Vesperini , D. Nardiello , D. Apai , A. J. Burgasser , R. Gerasimov , .

We present HST observations that show a bifurcation of colors in the middle main sequence of the globular cluster Omega Centauri. We see this in three different fields, observed with different cameras and filters. We also present high…

天体物理学 · 物理学 2009-10-05 L. R. Bedin , G. Piotto , J. Anderson , S. Cassisi , I. R. King , Y. Momany , G. Carraro , .

We present a Spitzer Space Telescope imaging survey of the most massive Galactic globular cluster, omega Centauri, and investigate stellar mass loss at low metallicity and the intracluster medium (ICM). The survey covers approximately 3.2x…

We investigate a peculiar feature at the hottest, blue end of the horizontal branch of Galactic globular cluster omega Centauri, using the high-precision and nearly complete catalog that has been constructed from a survey taken with the ACS…

太阳与恒星天体物理 · 物理学 2015-05-13 S. Cassisi , M. Salaris , J. Anderson , G. Piotto , A. Pietrinferni , A. Milone , A. Bellini , R. L. Bedin

We analyze the reddening, surface helium abundance and mass of 115 horizontal branch (HB) and blue hook (BH) stars in OmegaCentauri, spanning the HB from the blue edge of the instability strip to Teff~50000K. The mean cluster reddening is…

太阳与恒星天体物理 · 物理学 2015-06-11 C. Moni Bidin , S. Villanova , G. Piotto , S. Moehler , S. Cassisi , Y. Momany

In response to the proposed high helium content stars as an explanation for the double main sequence observed in Omega Centauri, we investigated the consequences of such stars elsewhere on the color-magnitude diagram. We concentrated on the…

天体物理学 · 物理学 2009-06-23 G. Newsham , D. M. Terndrup

We present an extensive photometry on HB, RGB, and MSTO stars in Omega Cen. The central regions of the cluster were covered with a mosaic of F435W, F625W, and F658N-band data collected with ACS/HST. The outer reaches were covered with a…

A direct measure of the helium abundances from the near-infrared transition of He I at 1.08 micron is obtained for two nearly identical red giant stars in the globular cluster Omega Centauri. One star exhibits the He I line; the line is…

太阳与恒星天体物理 · 物理学 2015-06-16 A. K. Dupree , E. H. Avrett

Recent studies suggest that the helium content of multiple stellar populations in globular clusters (GCs) is not uniform. The range of helium varies from cluster to cluster with more massive GCs having, preferentially, large helium spread.…

太阳与恒星天体物理 · 物理学 2015-06-23 A. P. Milone

Recent observational studies of $\omega$ Centauri by {\it Hubble Space Telescope} have discovered a double main sequence in the color magnitude diagrams (CMDs) of its stellar populations. The stellar population with the blue main sequence…

天体物理学 · 物理学 2009-11-13 Kenji Bekki , John E. Norris

Having shown in a recent paper that the main sequence of omega Centauri is split into two distinct branches, we now present spectroscopic results showing that the bluer sequence is_less_ metal-poor. We have carefully combined GIRAFFE@VLT…

In this paper we present the analysis of Hubble Space Telescope (HST) observations of the globular cluster Omega Centauri. Our analysis combines data obtained in this work with previously published HST data from an earlier article of this…

星系天体物理 · 物理学 2024-05-31 Michele Scalco , Luigi Bedin , Enrico Vesperini

Due to their extreme helium abundance, the multiple stellar populations of the globular cluster NGC 2808 have been widely investigated from a photometric, spectroscopic, and kinematic perspective. The most striking feature of the…

太阳与恒星天体物理 · 物理学 2016-08-11 Matteo Simioni , Antonino P. Milone , Luigi R. Bedin , Antonio Aparicio , Giampaolo Piotto , Enrico Vesperini , Jongsuk Hong

Deep HST-WFPC2 observations of the stellar population in the globular cluster Omega Cen (NGC 5139) have been used to measure the luminosity function of main sequence stars at the low-mass end. Two fields have been investigated, located…

天体物理学 · 物理学 2009-10-31 Guido De Marchi
‹ 上一页 1 2 3 10 下一页 ›