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相关论文: CHAOS III: Gas-Phase Abundances in NGC5457

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The CHemical Abundances of Spirals (CHAOS) project leverages the combined power of the Large Binocular Telescope (LBT) with the broad spectral range and sensitivity of the Multi Object Double Spectrograph (MODS) to measure "direct"…

We report the direct abundances for the galaxy NGC 2403 as observed by the CHemical Abundances Of Spirals (CHAOS) project. Using the Multi-Object Double Spectrograph on the Large Binocular Telescope, we observe two fields with H II regions…

The chemical abundances of spiral galaxies, as probed by HII regions across their disks, are key to understanding the evolution of galaxies over a wide range of environments. We present LBT/MODS spectra of 52 HII regions in NGC3184 as part…

We have observed NGC5194 (M51a) as part of the CHemical Abundances of Spirals (CHAOS) project. Using the Multi Object Double Spectrographs (MODS) on the Large Binocular Telescope (LBT) we are able to measure one or more of the…

星系天体物理 · 物理学 2015-08-06 Kevin V. Croxall , Richard W. Pogge , Danielle Berg , Evan D. Skillman , John Moustakas

The dispersion in chemical abundances provides a very strong constraint on the processes that drive the chemical enrichment of galaxies. Due to its proximity, the spiral galaxy M33 has been the focus of numerous chemical abundance surveys…

This paper presents a spectroscopic investigation of 11 HII regions in the nearby galaxy NGC 2403. The HII regions are observed with a long-slit spectrograph mounted on the 2.16 m telescope at XingLong station of National Astronomical…

星系天体物理 · 物理学 2018-02-14 Ye-Wei Mao , Lin Lin , Xu Kong

We present long-slit observations in the optical and near infrared of eight HII regions in the spiral galaxy NGC 4258. Six of the observed regions are located in the SE inner spiral arms and the other two are isolated in the northern outer…

天体物理学 · 物理学 2015-06-24 Angeles I. Diaz , Marcelo Castellanos , Elena Terlevich , Maria L. Garcia-Vargas

The CHAOS project is building a large database of LBT H II region spectra in nearby spiral galaxies to use direct abundances to better determine the dispersion in metallicity as a function of galactic radius. Here, we present CHAOS LBT…

(Abridged) We have obtained new spectrophotometric data for 28 HII regions in the spiral galaxy NGC 300, a member of the nearby Sculptor Group. The detection of auroral lines, including [OIII]4363, [SIII]6312 and [NII]5755, has allowed us…

宇宙学与河外天体物理 · 物理学 2009-07-22 Fabio Bresolin , Wolfgang Gieren , Rolf-Peter Kudritzki , Grzegorz Pietrzynski , Miguel A. Urbaneja , Giovanni Carraro

Spectroscopic observations of 63 HII regions in six spiral galaxies (NGC 628, NGC 783, NGC 2336, NGC 6217, NGC 7331, and NGC 7678) were carried out with the 6-meter telescope (BTA) of Russian Special Astrophysical Observatory with the…

宇宙学与河外天体物理 · 物理学 2012-06-21 Alexander S. Gusev , Leonid S. Pilyugin , Firouz Sakhibov , Sergey N. Dodonov , Olga V. Ezhkova , Maria S. Khramtsova

We investigate the chemical abundances of NGC3603 in the Milky Way, of 30Doradus in the Large Magellanic Cloud, and of N66 in the Small Magellanic Cloud. Mid-infrared observations with the Infrared Spectrograph onboard the Spitzer Space…

天体物理学 · 物理学 2009-11-13 V. Lebouteiller , J. Bernard-Salas , B. Brandl , D. G. Whelan , Y. Wu , V. Charmandaris , D. Devost , J. R. Houck

We present very deep spectrophotometry of 14 bright extragalactic HII regions belonging to spiral, irregular, and blue compact galaxies. The data for 13 objects were taken with the HIRES echelle spectrograph on the Keck I telescope. We have…

宇宙学与河外天体物理 · 物理学 2009-07-22 C. Esteban , F. Bresolin , M. Peimbert , J. Garcia-Rojas , A. Peimbert , A. Mesa-Delgado

Using deep Subaru/FOCAS spectra of 34 HII regions in both the inner and outer parts of the extended ultraviolet (XUV) disc galaxy NGC 4625 we have measured an abundance gradient out to almost 2.5 times the optical isophotal radius. We…

宇宙学与河外天体物理 · 物理学 2015-05-20 Q. E. Goddard , F. Bresolin , R. C. Kennicutt , E. V. Ryan-Weber , F. F. Rosales-Ortega

Gas-phase abundances provide insights into the baryon cycle, with radial gradients and 2D metallicity distributions tracking how metals build up and redistribute within galaxy disks over cosmic time. We use a catalog of 22,958 HII regions…

Motived by recent ISM studies, we present high quality MMT and Gemini spectroscopic observations of H II regions in the nearby spiral galaxies NGC 628 and NGC 2403 in order to measure their chemical abundance gradients. Using long-slit and…

Molecular line observations of NH3 (J,K)=(1,1), (2,2) and CH3OH at 24.93GHz taken with the Australian Telescope Compact Array (ATCA) toward the massive twin cores NGC6334 I & I(N) reveal significant variations in the line emission between…

天体物理学 · 物理学 2009-11-10 H. Beuther , S. Thorwirth , Q. Zhang , T. R. Hunter , S. T. Megeath , A. J. Walsh , K. M. Menten

The spectra of 413 star-forming (or HII) regions in M33 (NGC 598) were observed by using the multifiber spectrograph of Hectospec at the 6.5-m Multiple Mirror Telescope (MMT). By using this homogeneous spectra sample, we measured the…

星系天体物理 · 物理学 2017-06-20 Zesen Lin , Ning Hu , Xu Kong , Yulong Gao , Hu Zou , Enci Wang , Fuzhen Cheng , Guanwen Fang , Lin Lin , Jing Wang

Spectroscopic observations of 32 HII regions in the spiral galaxy NGC 3963 and the barred irregular galaxy NGC 7292 were carried out with the 2.5-m telescope of the Caucasus Mountain Observatory of the Sternberg Astronomical Institute using…

星系天体物理 · 物理学 2021-05-25 Alexander S. Gusev , Alexander V. Dodin

We present high signal-to-noise spectrophotometric observations of seven luminous HII galaxies. The observations have been made with the use of a double-arm spectrograph which provides spectra with a wide wavelength coverage, from 3400 to…

We present spectroscopic observations of a sample of 72 emission-line objects, including mainly HII regions, in the spiral galaxy M 33. Spectra were obtained with the multi-object, wide field spectrograph AF2/WYFFOS at the 4.2m WHT…

天体物理学 · 物理学 2009-11-13 L. Magrini , J. M. Vilchez , A. Mampaso , R. L. M. Corradi , P. Leisy
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