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相关论文: NGC 2915. II. A Dark Spiral Galaxy With A Blue Com…

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NGC 2915 is a nearby blue compact dwarf with the HI properties of a late-type spiral. Its large, rotating HI disk (extending out to R ~ 22 B-band scale lengths) and apparent lack of stars in the outer HI disk make it a useful candidate for…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. C. Elson , W. J. G. de Blok , R. C. Kraan-Korteweg

NGC 2915 is a blue compact dwarf galaxy embedded in an extended, low surface brightness HI disk exhibiting a two-armed spiral structure and a central bar-like component. Commonly accepted mechanisms are unable to explain the existence of…

天体物理学 · 物理学 2009-11-07 F. S. Masset , M. Bureau

NGC 2915 is a remarkable blue compact dwarf galaxy which contains an inner HI bar and strong spiral structure in its HI disk extending well beyond its optical disk. We propose here that NGC 2915 has a dark or faint (not yet observed)…

天体物理学 · 物理学 2007-05-23 A. C. Quillen

NGC 2915 is a blue compact dwarf galaxy with a very extended HI disk showing a short central bar and extended spiral arms, both reaching far beyond the optical component. We use Tremaine & Weinberg (1984) method to measure the pattern speed…

天体物理学 · 物理学 2009-10-31 M. Bureau , K. C. Freeman , D. W. Pfitzner , G. R. Meurer

The nearby blue compact dwarf, NGC 2915, has its stellar disc embedded in a large, extended (~ 22 B-band scale-lengths) HI disc. New high-resolution HI synthesis observations of NGC 2915 have been obtained with the Australia Telescope…

宇宙学与河外天体物理 · 物理学 2015-05-27 E. C. Elson , W. J. G. de Blok , R. C. Kraan-Korteweg

The HI disk of the blue compact dwarf (BCD) galaxy NGC 2915 extends to 22 optical scalelengths and shows spiral arms reaching far beyond the optical component. None of the previous theories for spiral structure provide likely explanations…

天体物理学 · 物理学 2016-08-30 Kenji Bekki , Kenneth C. Freeman

We present 21cm HI line observations of the blue compact dwarf galaxy NGC1705. Previous optical observations show a strong outflow powered by an ongoing starburst dominating the HII morphology and kinematics. In contrast, most of the HI…

天体物理学 · 物理学 2015-06-24 Gerhardt R. Meurer , Lister Staveley-Smith , N. E. B. Killeen

NGC 2915 is a nearby blue compact dwarf with a differentially rotating HI disc extending out to ~ 5 R-band R_{25} radii. This disc serves as an ideal tracer of the system's gravitational potential in regions of the galaxy that are dominated…

宇宙学与河外天体物理 · 物理学 2015-05-19 E. C. Elson , W. J. G. de Blok , R. C. Kraan-Korteweg

Results from new HI synthesis observations of the nearby blue compact dwarf galaxy, NGC 2915, carried out on the Australian Telescope Compact Array are presented. High resolution HI moment maps for the galaxy reveal complex HI distributions…

宇宙学与河外天体物理 · 物理学 2009-11-09 E. C. Elson , W. J. G. de Blok , R. C. Kraan-Koretweg

NGC 2915 is a unique nearby galaxy that is classified as an isolated blue compact dwarf based on its optical appearance but has an extremely extended H i gas disk with prominent Sd-type spiral arms. To unveil the starburst-triggering…

星系天体物理 · 物理学 2022-12-23 Yimeng Tang , Bojun Tao , Hong-Xin Zhang , Guangwen Chen , Yulong Gao , Zesen Lin , Yao Yao , Yong Shi , Xu Kong

We present new HI observations of the nearby dwarf galaxy NGC 3741. This galaxy has an extremely extended HI disk, which allows us to trace the rotation curve out to unprecedented distances in terms of the optical disk: we reach 42 B-band…

天体物理学 · 物理学 2008-11-26 G. Gentile , P. Salucci , U. Klein , G. L. Granato

We have discovered three globular clusters beyond the Holmberg radius in Hubble Space Telescope Advanced Camera for Surveys images of the gas-rich dark matter dominated blue compact dwarf galaxy NGC2915. The clusters, all of which start to…

Australia Telescope Compact Array HI-line observations of the nearby dwarf galaxy NGC 1705 are presented. The data are used to trace the gravitational potential of the galaxy out to several stellar disc scale lengths. A rotation curve is…

宇宙学与河外天体物理 · 物理学 2013-01-15 E. C. Elson , W. J. G. de Blok , R. C. Kraan-Korteweg

We exclude hydrogen burning stars, of any mass above the hydrogen-burning limit and any metallicity, as significant contributors to the massive halos deduced from rotation curves to dominate the outer parts of spiral galaxies. We present…

天体物理学 · 物理学 2009-10-30 Gerard Gilmore , M. Unavane

The Blue Compact Dwarf (BCD) galaxy SBS 0335--052 is one of the most metal--deficient galaxies known and one of the best candidates for a young dwarf galaxy in the process of formation. A VLA HI map reveals an unusual structure: the neutral…

We present a study of the HI distribution and dynamics of the nearby spiral galaxy NGC5055 based on observations with the Westerbork Synthesis Radio Telescope. The gaseous disk of NGC5055 extends out to about 40 kpc, equal to 3.5 R_25, and…

天体物理学 · 物理学 2009-11-11 G. Battaglia , F. Fraternali , T. Oosterloo , R. Sancisi

We have conducted a deep, complete HI survey, using Arecibo/ALFA, of a field centered on the nearby, isolated galaxy, NGC 2903, which is similar to the Milky Way in its properties. The field size was 150 kpc x 260 kpc and the final velocity…

Crucial to a quantitative understanding of galaxy evolution are the properties of the inter-stellar medium that regulate galactic-scale star formation activity. We present here the results of a suite of star formation models applied to the…

宇宙学与河外天体物理 · 物理学 2015-05-30 E C Elson , W J G de Blok , R C Kraan-Korteweg

Optical observations of Blue Compact Dwarf galaxies (BCDs) show they typically have high specific star formation rates and low metallicites. A subset of these galaxies (those with the lowest gas phase metallicities) display cometary optical…

星系天体物理 · 物理学 2025-01-06 Tom C. Scott , Elias Brinks , Chandreyee Sengupta , Patricio Lagos

We present HI observations of the elliptical galaxy NGC 2974, obtained with the Very Large Array. These observations reveal that the previously detected HI disc in this galaxy (Kim et al. 1988) is in fact a ring. By studying the harmonic…

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