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相关论文: Carbon and Oxygen Isotopic Ratios. II. Semiregular…

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C and O isotopic ratios are reported for a sample of 46 Mira and SRa-type variable AGB stars. Vibration-rotation 1st and 2nd overtone CO lines in 1.5 to 2.5 $\mu$m spectra were measured to derive isotopic ratios for 12C/13C, 16O/17O, and…

太阳与恒星天体物理 · 物理学 2016-07-06 K. H. Hinkle , T. Lebzelter , O. Straniero

We measured carbon abundances and the $^{12}\mathrm{C}/^{13}\mathrm{C}$ ratio in 31 giant branch stars with previous CN and CH band measurements that span -2.33 $<$ M$_{\rm V}$ $<$ 0.18 in the globular cluster M10 (NGC 6254). Abundances…

太阳与恒星天体物理 · 物理学 2019-06-14 Z. G. Maas , J. M. Gerber , Alex Deibel , C. A. Pilachowski

Context. The abundances of the three main isotopes of oxygen are altered in the course of the CNO-cycle. When the first dredge-up mixes the burning products to the surface, the nucleosynthesis processes can be probed by measuring oxygen…

太阳与恒星天体物理 · 物理学 2015-06-11 Thomas Lebzelter , Oscar Straniero , Kenneth Hinkle , Walter Nowotny , Bernhard Aringer

16O/17O and 12C/13C ratios in 23 M giants are determined from high resolution IR spectra observed with the KPNO FTS. The masses of our sample are estimated with the use of the evolutionary tracks by Claret (2004), which could account for…

天体物理学 · 物理学 2009-11-11 Takashi Tsuji

We present the first cross-identifications of sources in the near-infrared DENIS survey and in the micro-lensing EROS survey in a field of about 0.5 square degrees around the optical center (OC) of the Large Magellanic Cloud. We analyze the…

天体物理学 · 物理学 2009-11-07 M-R. L. Cioni , J-B. Marquette , C. Loup , M. Azzopardi , H. J. Habing , T. Lasserre , E. Lesquoy

Our understanding of large amplitude pulsating stars and their status in stellar evolution is briefly reviewed. The paper then describes the near-infrared light curves of various asymptotic giant branch stars, concentrating on possible…

天体物理学 · 物理学 2007-05-23 Patricia A. Whitelock

The 13-16 um region observed by the Infrared Space Observatory (ISO) of several ABG stars are discussed. We present and analyse spectra of seven M giants which show carbon dioxide features. To explain the features of the bands, we suggest…

天体物理学 · 物理学 2007-05-23 N. Ryde , K. Eriksson , B. Gustafsson

As part of a reanalysis of galactic Asymptotic Giant Branch (AGB) stars at infrared (IR) wavelengths, we discuss a sample (357) of carbon stars for which mass loss rates, near-IR photometry and distance estimates exist. For 252 sources we…

天体物理学 · 物理学 2016-08-30 R. Guandalini , M. Busso , S. Ciprini , G. Silvestro , P. Persi

Carbon-12 and carbon-13 abundances are measured in eleven red-giant members of the globular cluster Omega Centauri via observations of first-overtone CO bands near 2.3 microns. The mean value for the entire sample is <12C/13C>= 4.3 +/-0.4,…

天体物理学 · 物理学 2009-11-07 Verne V. Smith , Donald M. Terndrup , Nicholas B. Suntzeff

Fundamental parameters and the carbon, nitrogen and oxygen abundances are determined for 22 B-type stars with distances up to 600 pc and slow rotation (vsini up to 66 km/s). The stars are selected according to their effective temperatures…

太阳与恒星天体物理 · 物理学 2015-06-12 L. S. Lyubimkov , D. L. Lambert , D. B. Poklad , T. M. Rachkovskaya , S. I. Rostopchin

Previous determinations of the oxygen isotopic ratios in AGB carbon stars were at odds with the existing theoretical predictions. We aim to redetermine the oxygen ratios in these stars using new spectral analysis tools and further develop…

太阳与恒星天体物理 · 物理学 2017-03-08 Carlos Abia , Rubén P. Hedrosa , Inma Domínguez , Oscar Straniero

To search for phase lags in the optical-infrared light curves of asymptotic giant branch stars, we have compared infrared data from the COBE DIRBE satellite with optical light curves from the AAVSO and other sources. We found 17 examples of…

天体物理学 · 物理学 2008-11-26 Beverly J. Smith , Stephan D. Price , Amanda J. Moffett

Initial C/O ratios of circumstellar disks have been obtained in solar-type stars by differential photospheric abundance analysis with respect to the Sun. We present C/O ratios of M dwarfs obtained by absolute abundance analysis derived from…

太阳与恒星天体物理 · 物理学 2016-10-26 Tadashi Nakajima , Satoko Sorahana

We re-analysed the carbon and oxygen isotopic ratios in the atmospheres of the two bright K giants Arcturus and Aldebaran. Previous determinations of their 16O/18O ratios showed a rough agreement with FDU expectations; however, the…

太阳与恒星天体物理 · 物理学 2015-06-11 C. Abia , S. Palmerini , M. Busso , S. Cristallo

We report on oxygen abundances determined from medium-resolution near-IR spectroscopy for a sample of 57 carbon-enhanced metal-poor (CEMP) stars selected from the Hamburg/ESO survey. The majority of our program stars exhibit oxygen-to-iron…

As a byproduct of our search for Galactic stellar systems with gamma-ray emission, we have identified an unrelated cool and evolved star (IRC-10412) that attracted our attention due to its strong radio emission level with a spectral index…

太阳与恒星天体物理 · 物理学 2024-07-31 Pedro L. Luque-Escamilla , Josep Martí

We present angular size measurements of 22 oxygen-rich Mira variable stars. These data are part of a long term observational program using the Infrared Optical Telescope Array (IOTA) to characterize the observable behavior of these stars.…

天体物理学 · 物理学 2009-11-07 G. T. van Belle , R. R. Thompson , M. J. Creech-Eakman

Carbon- and Oxygen-rich stars populating the Thermally-Pulsing Asymptotic Giant Branch (TP-AGB) phase of stellar evolution are relevant contributors to the spectra of ~1 Gyr old populations. Atmosphere models for these types are uncertain,…

Optical radial velocities have been measured for 38 C-type Mira variables. These data together with others in the literature are used to study the differences between optical and CO mm observations for C-Miras and the necessary corrections…

天体物理学 · 物理学 2009-11-11 John W. Menzies , Michael W. Feast , Patricia A. Whitelock

We explore the ratio (C/M) of carbon-rich to oxygen-rich thermally pulsing asymptotic giant branch(TP-AGB) stars in the disk of M31 using a combination of moderate-resolution optical spectroscopy from the Spectroscopic Landscape of…

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