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相关论文: RRAB Variables and Metallicity

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The kinematic and Period-Luminosity-Colour distribution of O-rich Long-Period Variable stars of the solar neighbourhood is interpreted in terms of pulsation modes, masses and metallicities. It is first shown that, because of input physics…

天体物理学 · 物理学 2009-10-31 D. Barthes , X. Luri

This work presents the first long-term photometric variability survey of the intermediate-age open cluster NGC 559. Time-series V band photometric observations on 40 nights taken over more than three years with three different telescopes…

太阳与恒星天体物理 · 物理学 2020-09-30 Yogesh C. Joshi , Ancy Anna John , Jayanand Maurya , Alaxendra Panchal , Brijesh Kumar , Santosh Joshi

Stellar metallicity strongly correlates with the presence of planets and their properties. To check for new correlations between stars and the existence of an orbiting planet, we determine precise stellar parameters for a sample of…

太阳与恒星天体物理 · 物理学 2015-05-20 Sérgio G. Sousa , Nuno C. Santos , Garik Israelian , C. Lovis , Michel Mayor , Pedro B. Silva , Stephane Udry

We present a new detailed abundance study of field red horizontal branch (RHB) and blue horizontal branch (BHB) non-variable stars. High resolution and high S/N echelle spectra of 11 RHB and 12 BHB were obtained with the McDonald 2.7 m…

太阳与恒星天体物理 · 物理学 2015-05-20 Bi-Qing For , Christopher Sneden

The 3.6 and 4.5 micron characteristics of AGB variables in the LMC and IC1613 are discussed. For C-rich Mira variables there is a very clear period-luminosity-colour relation, where the [3.6]-[4.5] colour is associated with the amount of…

星系天体物理 · 物理学 2017-09-13 Patricia A. Whitelock , Mansi Kasliwal , Martha Boyer

New CCD photometry of NGC 6366 has lead to the discovery of some variable stars. Two possible Anomalous Cepheids (or Pop II Cepheids), three long period variables, one SX Phe and one eclipsing binary have been found. Also a list of 10…

天体物理学 · 物理学 2008-08-05 A. Arellano Ferro , Sunetra Giridhar , V. Rojas Lopez , R. Figuera , D. M. Bramich , P. Rosenzweig

The ground-based Konkoly Blazhko Survey I and II aim to collect accurate, extended, multicolour light curves of galactic field RRab stars in order to determine the incidence rate of the modulation in the sample, to study the modulation in…

太阳与恒星天体物理 · 物理学 2011-01-27 Ádám Sódor

Constraints on the Galactic bulge/bar structure and formation history from stellar kinematics and metallicities mainly come from relatively high-latitude fields (|b|>4) where a complex mix of stellar population is seen. We aim here to…

We present new nonlinear, time-dependent convective hydrodynamical models of RR Lyrae stars computed assuming a constant helium-to-metal enrichment ratio and a broad range in metal abundances (Z=0.0001--0.02). The stellar masses and…

太阳与恒星天体物理 · 物理学 2015-08-06 M. Marconi , G. Coppola , G. Bono , V. Braga , A. Pietrinferni , R. Buonanno , M. Castellani , I. Musella , V. Ripepi , R. F. Stellingwerf

We present a detailed spectroscopic analysis of nitrogen abundances in 91 solar-type stars, 66 with and 25 without known planetary mass companions. All comparison sample stars and 28 planet hosts were analysed by spectral synthesis of the…

天体物理学 · 物理学 2016-08-16 A. Ecuvillon , G. Israelian , N. C. Santos , M. Mayor , R. J. García López , S. Randich

The light curves of 50 RRab (RR0) stars in M5 collected in Paper I are investigated to detect Blazhko modulation. 18 Blazhko stars are identified, and modulation is suspected in two additional cases. The mean pulsation period of Blazhko…

太阳与恒星天体物理 · 物理学 2015-05-20 J. Jurcsik , B. Szeidl , C. Clement , Zs. Hurta , M. Lovas

RR Lyrae stars pulsating in the fundamental mode have long been used to measure interstellar reddening, based on their observed uniformity of $B-V$ color at minimum light after small corrections for metallicity and period are applied.…

太阳与恒星天体物理 · 物理学 2013-10-03 Andrew Layden , Tyler Anderson , Paul Husband

Results of a search for variable stars in the central region of the globular cluster M13 are presented. Prior to this study, 36 variable and suspected variable stars were known in this cluster (Osborn 2000; Clement et al. 2001). Of these…

天体物理学 · 物理学 2009-11-07 G. Kopacki , Z. Kolaczkowski , A. Pigulski

We investigate the Milky Way Galaxy's radial and vertical metallicity gradients using a sample of 47,406 red clump stars from the RAVE DR4. This sample is more than twice the size of the largest sample in the literature investigating radial…

星系天体物理 · 物理学 2016-09-28 O. Onal Tas , S. Bilir , G. M. Seabroke , S. Karaali , S. Ak , T. Ak , Z. F. Bostanci

Analysis of cluster and field star uvby data demonstrates the existence of a previously undetected discrepancy in a widely used photometric metallicity calibration for G dwarfs. The discrepancy is systematic and strongly color-dependent,…

天体物理学 · 物理学 2009-11-07 Bruce A. Twarog , Barbara J. Anthony-Twarog , Delora Tanner

Context. Reliable metallicity values for M dwarfs are important for studies of the chemical evolution and advancement of planet formation theory in low-mass environments. Historically the determination of stellar parameters of low-mass…

太阳与恒星天体物理 · 物理学 2017-08-16 Sara Lindgren , Ulrike Heiter

We present recent results from our radial velocity (RV) studies of rapidly oscillating Ap (roAp) stars. Our measurements reveal that the pulsational amplitude of these stars depends on the spectral region that is examined. For one star,…

天体物理学 · 物理学 2007-05-23 A. P. Hatzes , A. Kanaan

We present here the first observation of galactic AGB stars with the InfraRed Array Camera (IRAC) onboard the Spitzer Space Telescope. Our sample consists of 48 AGB stars of different chemical signature, mass loss rate and variability…

天体物理学 · 物理学 2009-06-23 Massimo Marengo , Megan Reiter , Giovanni G. Fazio

Luminous Blue Variables are massive evolved stars, here we introduce this outstanding class of objects. Described are the specific characteristics, the evolutionary state and what they are connected to other phases and types of massive…

太阳与恒星天体物理 · 物理学 2020-09-08 Kerstin Weis , Dominik J. Bomans

We have carried out a search for new R Coronae Borealis (RCB) variables using the publicly accessible data from various photometric sky surveys and-whenever available-AAVSO visual data. Candidates were selected from Tisserand`s "Catalogue…

太阳与恒星天体物理 · 物理学 2014-06-26 Sebastián Otero , Stefan Huemmerich , Klaus Bernhard , Igor Soszyński