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相关论文: Dust and Super Star Clusters in NGC 5253

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Hidden from optical view in the starburst region of the dwarf galaxy NGC 5253 lies an intense radio source with an unusual spectrum which could be interpreted variously as nebular gas ionized by a young stellar cluster or nonthermal…

天体物理学 · 物理学 2009-11-06 Varoujan Gorjian , Jean L. Turner , Sara C. Beck

We present observations of a massive star cluster near the nuclear region of the nearby starburst galaxy NGC 253. The peak of near-infrared emission, which is spatially separated by 4" from the kinematic center of the galaxy, is coincident…

太阳与恒星天体物理 · 物理学 2010-01-15 Katherine A. Kornei , Nate McCrady

The nearby dwarf starburst galaxy NGC5253 hosts a number of young, massive star clusters, the two youngest of which are centrally concentrated and surrounded by thermal radio emission (the `radio nebula'). To investigate the role of these…

The blue compact dwarf galaxy NGC 5253 hosts a very young central starburst. The center contains intense radio thermal emission from a massive ultracompact H II region (or "supernebula") and two massive and very young super star clusters…

星系天体物理 · 物理学 2020-06-24 Linda J. Smith , Varun Bajaj , Jenna Ryon , Elena Sabbi

A giant molecular cloud has been detected surrounding the supernebula in NGC 5253, revealing details of the formation and feedback process in a very massive star cluster. "Cloud D" was recently mapped in CO J=3-2 with the Submillimeter…

星系天体物理 · 物理学 2015-09-30 Jean L. Turner

Using high-resolution Hubble Space Telescope data, we reexamine the fundamental properties (ages, masses and extinction values) of the rich star cluster population in the dwarf starburst galaxy NGC 5253. The gain in resolution compared to…

宇宙学与河外天体物理 · 物理学 2015-06-15 Richard de Grijs , Peter Anders , Erik Zackrisson , Göran Östlin

We report the detection of CO(2-1) and 3.1 mm and 1.3 mm continuum emission towards the extremely young starburst in NGC 5253, with data taken from the Owens Valley Millimeter Array. Faint CO emission originates in five molecular clouds…

天体物理学 · 物理学 2009-11-07 David S. Meier , Jean L. Turner , Sara C. Beck

NGC 253 hosts the nearest nuclear starburst. Previous observations show a region rich in molecular gas, with dense clouds associated with recent star formation. We used ALMA to image the 350 GHz dust continuum and molecular line emission…

We present a detailed analysis of the star cluster population in the starburst galaxy NGC 5253. Our work is based on HST optical and VLT Ks images. We detect more than 300 clusters, and for all of them we derive the photometry in the V, I…

天体物理学 · 物理学 2009-11-10 G. Cresci , L. Vanzi , M. Sauvage

Subarcsecond infrared and radio observations yield important information about the formation of super star clusters from their surrounding gas. We discuss the general properties of ionized and molecular gas near young, forming SSCs, as…

天体物理学 · 物理学 2007-05-23 Jean L. Turner , Sara C. Beck

A local dwarf galaxy, NGC 5253, has a young super star cluster that may provide an example of highly efficient star formation. Here we report the detection and imaging, with the Submillimeter Array, of the J= 3-2 rotational transition of CO…

星系天体物理 · 物理学 2015-03-19 J. L. Turner , S. C. Beck , D. J. Benford , S. M. Consiglio , P. T. P. Ho , A. Kovács , D. S. Meier , J. -H. Zhao

Young massive clusters play an important role in the evolution of their host galaxies, and feedback from the high-mass stars in these clusters can have profound effects on the surrounding interstellar medium. The nuclear starburst in the…

We investigate the star cluster population in the outer parts of the starburst galaxy NGC 5253 using archive images taken with the Hubble Space Telescope's Advanced Camera for Surveys. Based on the F415W, F555W, and F814W photometry ages…

宇宙学与河外天体物理 · 物理学 2015-06-04 D. Harbeck , J. Gallagher , D. Crnojević

The blue compact dwarf galaxy NGC 5253 hosts a very young starburst containing twin nuclear star clusters, separated by a projected distance of 5 pc. One cluster (#5) coincides with the peak of the H-alpha emission and the other (#11) with…

星系天体物理 · 物理学 2016-06-01 L. J. Smith , P. A. Crowther , D. Calzetti , F. Sidoli

A 180 micron map and strip maps at 120 and 180 microns were obtained for the edge-on starburst galaxy NGC 253 with ISOPHOT, the photometer on board the Infrared Space Observatory. We compare these observations with those obtained by IRAS at…

天体物理学 · 物理学 2009-11-07 M. Radovich , J. Kahanpaa , D. Lemke

We investigate the star formation history of both the bright star clusters and the diffuse `field star' population in the dwarf starburst galaxy NGC 5253 using STIS longslit ultraviolet spectroscopy. Our slit covers a physical area of 370 x…

天体物理学 · 物理学 2009-11-06 C. A. Tremonti , D. Calzetti , C. Leitherer , T. M. Heckman

NGC 253 is a nearby spiral galaxy that is currently undergoing a nuclear burst of star formation in a 100 pc diameter region. We present spatially resolved 8--13 micron low-resolution spectra at four positions along the ridge of 8--13…

天体物理学 · 物理学 2009-10-31 C. C. Dudley , C. G. Wynn-Williams

NGC 5253 is a nearby (D=3.6 Mpc) Blue Compact Dwarf galaxy, notable for its three massive young super star clusters (SSCs) and nitrogen enrichment. Its similarity to extreme star-forming galaxies at high redshift makes it a good local…

The nearby dwarf starburst NGC 5253 is dominated by a compact radio-infrared supernebula powered by a very young and bright embedded Super Star Cluster (SSC) of $\sim 10^9 L_\odot$. We observed this source and its surroundings over the…

Little is known about the origins of the giant star clusters known as globular clusters. How can hundreds of thousands of stars form simultaneously in a volume only a few light years across the distance of the sun to its nearest neighbor?…

天体物理学 · 物理学 2015-06-24 J. L. Turner , S. C. Beck , L. P. Crosthwaite , J. E. Larkin , I. S. McLean , D. S. Meier
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