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相关论文: SDSS J170745+302056: a low surface brightness gala…

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We serendipitously find a new nearby Low Surface Brightness (LSB) galaxy from SDSS database. We estimate oxygen abundance of its H II region SDSS J121811.0+465501.2 from electron temperature, as well as for another H II region, SDSS…

天体物理学 · 物理学 2008-11-26 Y. C. Liang , J. Y. Hu , F. S. Liu , Z. T. Liu

Highly magnified lensed galaxies allow us to probe the morphological and spectroscopic properties of high-redshift stellar systems in great detail. However, such objects are rare, and there are only a handful of lensed galaxies which are…

天体物理学 · 物理学 2009-11-13 Eran O. Ofek , Stella Seitz , Felix Klein

We provide evidence that UGC1382, long believed to be a passive elliptical galaxy, is actually a giant low surface brightness (GLSB) galaxy which rivals the archetypical GLSB Malin 1 in size. Like other GLSB galaxies, it has two components:…

We present the first result of a survey for strong galaxy-galaxy lenses in Sloan Digital Sky Survey (SDSS) images. SDSS J082728.70+223256.4 was selected as a lensing candidate using selection criteria based on the color and positions of…

We report the discovery of a rare compact early-type galaxy, SDSS J085431.18+173730.5 (hereafter cE\_AGN). It has an half light radius of R$_{e}$ = 490 pc and a brightness of M$_{r}$ = $-$18.08 mag. Optical spectroscopy available from the…

星系天体物理 · 物理学 2016-04-06 Sanjaya Paudel , Michael Hilker , Change Hee Ree , Minjin Kim

We present the results of observations of the very low surface brightness (VLSB) dwarf galaxy SDSS J092609.45+334304.1 with extreme parameters which indicate its unevolved status. Namely, its value of O/H, derived as an average of that in…

宇宙学与河外天体物理 · 物理学 2015-05-14 S. A. Pustilnik , A. L. Tepliakova , A. Y. Kniazev , J. -M. Martin , A. N. Burenkov

Scaling relations are fundamental tools for exploring the morphological properties of galaxies and understanding their formation and evolution. Typically, galaxies follow a scaling relation between mass and size, measured by effective…

We report the discovery of SDSSJ1049+5103, an overdensity of resolved blue stars at (\alpha_{2000}, \delta_{2000}) = (162.343, 51.051). This object appears to be an old, metal-poor stellar system at a distance of 45 +/- 10 kpc, with a…

For lensed galaxy SGAS J111020.0+645950.8 at redshift z=2.481, which is magnified by a factor of 28 +- 8, we analyze the morphology of star formation as traced by rest-frame ultraviolet emission, in both the highly-magnified source plane,…

星系天体物理 · 物理学 2017-07-19 J. R. Rigby , T. L. Johnson , K. Sharon , K. Whitaker , M. D. Gladders , M. Florian , J. Lotz , M. Bayliss , E. Wuyts

We have obtained optical spectroscopy of one of the most metal-poor dwarf star-forming galaxies (SFG) in the local Universe, J1234+3901, with the Large Binocular Telescope (LBT)/Multi-Object Dual Spectrograph (MODS). This blue compact dwarf…

星系天体物理 · 物理学 2019-03-01 Y. I. Izotov , T. X. Thuan , N. G. Guseva

We present properties of the low-surface-brightness galaxy KDG 218 observed with the HST/ACS. The galaxy has a half-light (effective) diameter of $a_e =47^{\prime\prime}$ and a central surface brightness of $SB_V(0) =…

星系天体物理 · 物理学 2017-12-13 I. D. Karachentsev , L. N. Makarova , M. E. Sharina , V. E. Karachentseva

A large sample of low surface brightness (LSB) disk galaxies is selected from SDSS with B-band central surface brightness mu_0(B) from 22 to 24.5 mag arcsec^(-2). Some of their properties are studied, such as magnitudes, surface brightness,…

宇宙学与河外天体物理 · 物理学 2015-05-14 Y. C. Liang , G. H. Zhong , X. Y. Chen , D. Gao , F. Hammer , F. S. Liu , J. Y. Hu , L. C. Deng , B. Zhang

We present our discovery of a complex ionized outflow in SDSS J101034.28+372514.7 (J1010+3725), a dust-obscured galaxy (DOG) at $z=0.282$. The SDSS optical spectrum of J1010+3725 shows five narrow components with one broad component in…

星系天体物理 · 物理学 2026-05-14 Taketo Yoshida , Tohru Nagao , Yoshiki Toba , Naomichi Yutani , Thomas Bohn , Kohei Shibata , Nozomu Tamada

SDSS J0015+0104 is the lowest metallicity low surface brightness dwarf (LSBD) galaxy known. The oxygen abundance in its HII region SDSS J001520.70+010436.9 (at ~1.5 kpc from the galaxy centre) is 12+log(O/H)=7.07 (Guseva et al.). This…

宇宙学与河外天体物理 · 物理学 2015-06-15 S. A. Pustilnik , J. -M. Martin , Y. A. Lyamina , A. Y. Kniazev

We report the discovery of an intriguing, low-mass galaxy-scale strong-lens system in the SMACS J0723.3-7327 galaxy cluster. By modeling James Webb Space Telescope imaging and Very Large Telescope Multi-Unit Spectroscopic Explorer…

星系天体物理 · 物理学 2025-04-28 Limeng Deng , Yiping Shu , Lei Wang , Guoliang Li , Gabriel Bartosch Caminha , Jiang Dong , Zizhao He , Han Qu , Ruibiao Luo

Detailed analyses of high-redshift galaxies are challenging due to their faintness, but this difficulty can be overcome with gravitational lensing, in which the magnification of the flux enables high signal-to-noise ratio (S/N)…

星系天体物理 · 物理学 2021-12-08 Annalisa Citro , Dawn K. Erb , Max Pettini , Matthew W. Auger , George D. Becker , Bethan L. James

We report the discovery of a high proper motion L subdwarf ($\mu$ =0.617arcsec/yr) in the Sloan Digital Sky Survey spectral database. The optical spectrum from the star SDSS J125637-022452 has mixed spectral features of both late-M spectral…

太阳与恒星天体物理 · 物理学 2009-11-13 T. Sivarani , S. Lépine , A. K. Kembhavi , J. Gupchup

We present measurements of the surface density of star formation, the star-forming clump luminosity function, and the clump size distribution function, for the lensed galaxy SGAS J111020.0+645950.8 at a redshift of z=2.481. The physical…

We report the discovery of an isolated compact galaxy triplet SDSS J084843.45+164417.3, which is first detected by the LAMOST spectral survey and then confirmed by the spectroscopic observation of the BFOSC of the 2.16 meter telescope. It…

星系天体物理 · 物理学 2016-05-25 Shuai Feng , Zheng-Yi Shao , Shi-Yin Shen , Maria Argudo-Fernández , Hong Wu , Man-I Lam , Ming Yang , Fang-Ting Yuan

UGC 12281 has been classified as having a pure disk and being a low surface brightness galaxy (LSBG), thus being an obvious member of the so-called superthin galaxies. At the same time it represents an extremely untypical type of LSBG due…

星系天体物理 · 物理学 2015-06-03 Philip Günster , Dominik J. Bomans
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