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Related papers: Oxygen abundance distribution in Galactic disc

200 papers

We derived elemental abundances in 27 Cepheids, the great majority situated within a zone of Galactocentric distances ranging from 5 to 7 kpc. One star of our sample, SU Sct, has a Galactocentric distance of about 3 kpc, and thus falls in a…

Astrophysics of Galaxies · Physics 2015-06-24 R. P. Martin , S. M. Andrievsky , V. V. Kovtyukh , S. A. Korotin , I. A. Yegorova , Ivo Saviane

We present spectra obtained with the 10.4 m Gran Telescopio Canarias telescope of 13 Galactic HII regions, most of them of very low ionisation degree. The objects are located along the Galactic disc, with R_G from 5.7 to 16.1 kpc. We…

Astrophysics of Galaxies · Physics 2018-05-16 C. Esteban , J. Garcia-Rojas

Oxygen abundances for a large sample of dwarf and giant stars kinematically selected to be part of the Galactic thin and thick disks have been determined from a non-LTE analysis of the O I triplet lines at 777 nm. The abundance analysis was…

Astrophysics · Physics 2009-11-11 I. Ramirez , C. Allende Prieto , D. L. Lambert

Spectra of 34 H II regions in the late-type galaxies NGC1087, NGC2967, NGC3023, NGC4030, NGC4123, and NGC4517A were observed with the South African Large Telescope (SALT). In all 34 H II regions, oxygen abundances were determined through…

Astrophysics of Galaxies · Physics 2015-10-07 I. A. Zinchenko , A. Y. Kniazev , E. K. Grebel , L. S. Pilyugin

We investigate the oxygen and nitrogen abundance distributions across the optical disks of 130 nearby late-type galaxies using around 3740 published spectra of HII regions. We use these data in order to provide homogeneous abundance…

Astrophysics of Galaxies · Physics 2015-06-19 L. S. Pilyugin , E. K. Grebel , A. Y. Kniazev

We have obtained deep multi-object optical spectra of 49 HII regions in the outer disk of the spiral galaxy M83 (=NGC 5236) with the FORS2 spectrograph at the Very Large Telescope. The targets span the range in galactocentric distance…

Astrophysics of Galaxies · Physics 2011-02-11 Fabio Bresolin , Emma Ryan-Weber , Robert C. Kennicutt , Quinton Goddard

We characterise the oxygen abundance radial distribution of a sample of 102 spiral galaxies observed with VLT/MUSE using the O3N2 calibrator. The high spatial resolution of the data allows us to detect 14345 HII regions with the same image…

The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby (d<150 pc) FGK disk and halo stars with metallicities in the range -1.5<[Fe/H]<0.5. The oxygen abundances were inferred from a restricted non-LTE…

Astrophysics · Physics 2009-11-13 I. Ramirez , C. Allende Prieto , D. L. Lambert

First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented. Oxygen abundances for 21 thick disk and 42 thin disk F and G dwarf stars based on very high resolution spectra (R\sim 215000)…

Astrophysics · Physics 2007-05-23 T. Bensby , S. Feltzing , I. Lundstrom

We measured the gas abundance profiles in a sample of 122 face-on spiral galaxies observed by the CALIFA survey and included all spaxels whose line emission was consistent with star formation. This type of analysis allowed us to improve the…

First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented. Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high…

Astrophysics · Physics 2010-04-28 T. Bensby , S. Feltzing , I. Lundström

We use the EAGLE simulations to study the oxygen abundance gradients of gas discs in galaxies within the stellar mass range [10^9.5, 10^10.8]Mo at z=0. The estimated median oxygen gradient is -0.011 (0.002) dex kpc^-1, which is shallower…

We present deep optical spectroscopy of eight HII regions located in the anticentre of the Milky Way. The spectra were obtained at the 10.4m GTC and 8.2m VLT. We determined Te([NII]) for all objects and Te([OIII]) for six of them. We also…

Astrophysics of Galaxies · Physics 2017-08-16 C. Esteban , X. Fang , J. Garcia-Rojas , L. Toribio San Cipriano

Using a sample of 31 main-sequence OB stars located between galactocentric distances 8.4 - 15.6 kpc, we aim to probe the present-day radial abundance gradients of the Galactic disk. The analysis is based on high-resolution spectra obtained…

Solar and Stellar Astrophysics · Physics 2019-05-29 G. A. Braganca , S. Daflon , T. Lanz , K. Cunha , T. Bensby , P. J. McMillan , C. D. Garmany , J. W. Glaspey , M. Borges Fernandes , M. S. Oey , I. Hubeny

We present oxygen abundances for 72 F and G dwarf stars in the solar neighbourhood. Using the kinematics of the stars we divide them into two sub-samples with space velocities that are typical for the thick and thin disks, respectively. The…

Astrophysics · Physics 2009-11-10 T. Bensby , S. Feltzing , I. Lundstrom

The well-observed spiral galaxy M101 was considered. The radial distributions of oxygen abundances determined in three different ways (with the classic Te - method, with the R23 - method, and with the P -- method) were compared. It was…

Astrophysics · Physics 2009-11-06 L. S. Pilyugin

We determine the radial abundance gradient of helium in the disc of the Galaxy from published spectra of 19 $\text{H}\thinspace \text{II}$ regions and ring nebulae surrounding massive O stars. We revise the Galactocentric distances of the…

Solar and Stellar Astrophysics · Physics 2020-06-16 J. E. Méndez-Delgado , C. Esteban , J. García-Rojas , K. Z. Arellano-Córdova , M. Valerdi

We have obtained spectrophotometric observations of 41 anticenter planetary nebulae (PNe) located in the disk of the Milky Way. Electron temperatures and densities, as well as chemical abundances for He, N, O, Ne, S, Cl, and Ar were…

We analyse the global structure of the old stellar discs in 34 edge-on spiral galaxies. The radial and vertical exponential scale parameters of the discs are obtained by applying an improved two-dimensional decomposition technique to our…

Astrophysics · Physics 2009-11-07 Michiel Kregel , Pieter C. van der Kruit , Richard de Grijs

We consider the oxygen abundance distributions for a sample of massive spiral galaxies from the MaNGA survey in which the radial abundance gradient flattens to a constant value outside of the outer break radius, Rb,outer. The outer break…

Astrophysics of Galaxies · Physics 2026-01-08 L. S. Pilyugin , G. Tautvaisiene
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