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相关论文: Unusual void galaxy DDO68: implications of the HST…

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We present the results of optical spectroscopy and imaging with the SAO 6m telescope for the dwarf galaxy DDO 68 (UGC 5340 = VV 542), falling into the region of very low density of luminous (L > L*) galaxies (Lynx-Cancer void). Its deep…

天体物理学 · 物理学 2009-11-11 S. A. Pustilnik , A. Y. Kniazev , A. G. Pramskij

We present the star formation history of the extremely metal-poor dwarf galaxy DDO 68, based on our photometry with the Advanced Camera for Surveys. With a metallicity of only $12+\log(O/H)=7.15$ and a very isolated location, DDO 68 is one…

星系天体物理 · 物理学 2016-10-12 E. Sacchi , F. Annibali , M. Cignoni , A. Aloisi , T. Sohn , M. Tosi , R. P. van der Marel , A. J. Grocholski , B. James

DDO 68 is the second most metal-poor star-forming galaxy (12+log(O/H)=7.14). Its peculiar optical morphology and the data on its HI distribution and kinematics indicate the merger origin. We use the photometry of the SDSS u,g,r,i images of…

天体物理学 · 物理学 2007-12-27 S. A. Pustilnik , A. L. Tepliakova , A. Y. Kniazev

The paper presents new results of the ongoing study of the unusual Lynx-Cancer void galaxy DDO 68 with record-low-metallicity regions (12+log(O/H) ~7.14) of the current star formation (SF). They include: a) a new spectrum and photometry…

星系天体物理 · 物理学 2016-11-28 S. A. Pustilnik , L. N. Makarova , Y. A. Perepelitsyna , A. V. Moiseev , D. I. Makarov

We present the results of deep Hubble Space Telescope photometry of the dwarf galaxy DDO 68-C, proposed as possibly associated with the isolated peculiar dwarf DDO 68. The new data resolve for the first time the stars of DDO 68-C down to…

We present HI spectral-line imaging of the extremely metal-poor galaxy DDO 68. This system has a nebular oxygen abundance of only 3% Z$_{\odot}$, making it one of the most metal-deficient galaxies known in the local volume. Surprisingly,…

We present new Hubble Space Telescope (HST) imaging of a stream-like system associated with the dwarf galaxy DDO 68, located in the Lynx-Cancer Void at a distance of D$\sim$12.65 Mpc from us. The stream, previously identified in deep Large…

星系天体物理 · 物理学 2019-09-25 F. Annibali , M. Bellazzini , M. Correnti , E. Sacchi , M. Tosi , M. Cignoni , A. Aloisi , D. Calzetti , L. Ciotti , F. Cusano , J. Lee , C. Nipoti

Through adaptive optics (AO) imaging with the SOUL+LUCI instrument at the Large Binocular Telescope we were able to resolve, for the first time, individual stars in the gas-rich galaxy DDO68 C. This system was already suggested to be…

DDO68 is a star-forming (SF) dwarf galaxy residing in a nearby void. Its gas metallicity is among the lowest known in the local Universe, with parameter 12+log(O/H) in the range of 6.96-7.3 dex. Six of its SF regions are located in or near…

Here we present observations with the Advanced Camera for Surveys on the Hubble Space Telescope of the nearby, transition-type dwarf galaxy KK258 = ESO468-020. We measure a distance of 2.23$\pm$0.05 Mpc using the Tip of Red Giant Branch…

星系天体物理 · 物理学 2015-06-22 I. D. Karachentsev , L. N. Makarova , R. B. Tully , Po-Feng Wu , A. Y. Kniazev

We present chemical abundances and radial velocities of six HII regions in the extremely metal-poor star-forming dwarf galaxy DDO 68. They are derived from deep spectra in the wavelength range 3500 - 10,000 {\AA}, acquired with the Multi…

The lowest metallicity massive stars in the Local Universe with Z~(Zo/50-Zo/30) are the crucial objects to test the validity of assumptions in the modern models of very low-metallicity massive star evolution. These models, in turn, have…

星系天体物理 · 物理学 2020-01-08 Yulia Perepelitsyna , Simon Pustilnik

We present sensitive and high resolution 21 cm observations of the dwarf irregular (dIm) galaxy DDO 43, in conjunction with optical broad and narrow band images in U, B, V, and Halpha. The observations are used to examine the relationship…

天体物理学 · 物理学 2008-11-26 Caroline E. Simpson , Deidre A. Hunter , Tyler E. Nordgren

We present new photometry of the dwarf irregular galaxy DDO 68, one of the most metal-poor and least massive dwarfs, located in the Lynx-Cancer Void. The images were acquired with the Large Binocular Telescope in the g and r passbands, and…

星系天体物理 · 物理学 2016-08-17 F. Annibali , C. Nipoti , L. Ciotti , M. Tosi , A. Aloisi , M. Bellazzini , M. Cignoni , F. Cusano , D. Paris , E. Sacchi

We use Subaru Suprime-Cam and VLT FORS1 photometry of the dwarf galaxy DDO210 to study the global stellar content and structural properties of a transition-type galaxy (with properties intermediate between dwarf irregular and dwarf…

天体物理学 · 物理学 2009-11-11 Alan W. McConnachie , Nobuo Arimoto , Mike Irwin , Eline Tolstoy

We present HI 21cm and optical observations of UGC 3672 which is located near the centre of the nearby Lynx-Cancer void. We find that UGC 3672 consists of an approximately linearly aligned triplet of gas rich dwarfs with large scale…

星系天体物理 · 物理学 2017-01-18 Jayaram N. Chengalur , S. A. Pustilnik , E. S. Egorova

We present a quantitative star formation history of the nearby dwarf galaxy UGCA 92. This irregular dwarf is situated in the vicinity of the Local Group of galaxies in a zone of strong Galactic extinction (IC 342 group of galaxies). The…

宇宙学与河外天体物理 · 物理学 2015-06-04 Lidia Makarova , Dmitry Makarov , Sergey Savchenko

We present an HI and optical study of the gas-rich dwarf irregular galaxy DDO 88. Although DDO 88's global optical and HI parameters are normal for its morphological type, it hosts a large (3 kpc diameter) and unusually complete ring of…

天体物理学 · 物理学 2009-11-10 Caroline E. Simpson , Deidre A. Hunter , Patricia M. Knezek

We present Giant Metrewave Radio Telescope (GMRT) observations for three (viz., DDO 68, SDSS J2104-0035 and UGC 772) of the six most metal-deficient actively star-forming galaxies known. Although there is a debate as to whether these…

天体物理学 · 物理学 2009-11-13 Ekta , Jayaram N. Chengalur , S. A. Pustilnik

The Local Volume dwarf galaxy DDO 68, from the spectroscopy of its two brightest HII regions (Knots 1 and 2) was designated as the second most metal-poor star-forming galaxy [12+log(O/H)=7.14]. In the repeated spectral observations in 2008…

天体物理学 · 物理学 2009-11-13 S. A. Pustilnik , A. L. Tepliakova , A. Y. Kniazev , A. N. Burenkov
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