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相关论文: Direct detection of galaxy stellar halos : NGC 395…

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We present H-band images obtained with NICMOS of a field 75'' (5kpc) above the plane of the disk of the edge-on spiral galaxy NGC 5907. Ground-based observations have shown that NGC 5907 has a luminous halo with a shallow radial profile…

天体物理学 · 物理学 2009-10-31 Stephen E. Zepf , Michael C. Liu , Francine R. Marleau , Penny D. Sackett , James. R. Graham

Using long exposures taken in the V and I bands with a 4096$\times$4096 pixel CCD array at the prime focus of the Canada-France-Hawaii telescope, we have confirmed the discovery by Sackett et al. (1994) of a flat, faint luminous halo around…

天体物理学 · 物理学 2019-08-15 J. Lequeux , B. Fort , M. Dantel-Fort Fort , J. -C. Cuillandre , Y. Mellier , M. Dantel-Fort Fort

We present the preliminary detection of a stellar halo in the nearby, edge-on galaxy, NGC 4244. Using data from the Hubble Space Telescope's Advanced Camera for Surveys (HST/ACS), we have examined number counts of red giant branch (RGB)…

天体物理学 · 物理学 2009-11-13 Anil Seth , Roelof De Jong , Julianne Dalcanton , the GHOSTS team

We present a search for near-infrared (3.5-5 micron) emission from baryonic dark matter in the form of low-mass stars and/or brown dwarfs in the halo of the nearby edge-on spiral galaxy NGC 5907. The observations were made using a 256 by…

天体物理学 · 物理学 2009-10-31 S. A. Yost , J. J. Bock , M. Kawada , A. E. Lange , T. Matsumoto , K. Uemizu , T. Watabe , T. Wada

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

We report optical photometry and HI synthesis observations of the southern edge-on S_c,d galaxy IC5249. The observations were carried out primarily to determine if IC5249 has a red halo surrounding it similar to the halo that has been…

天体物理学 · 物理学 2012-08-27 The MOA Collaboration

The extended stellar halos of galaxies contain important clues for investigating their assembly history and evolution. We investigate the resolved stellar content and the extended halo of NGC 5128 as a function of galactocentric distance.…

星系天体物理 · 物理学 2022-01-05 M. Rejkuba , W. E. Harris , L. Greggio , D. Crnojević , G. L. H. Harris

The stellar haloes of galaxies can currently be studied either through observations of resolved halo stars or through surface photometry. Curiously, the two methods appear to give conflicting results, as a number of surface photometry…

宇宙学与河外天体物理 · 物理学 2015-06-03 E. Zackrisson , R. S. de Jong , G. Micheva

We use a sample of 17 strong gravitational lens systems from the BELLS GALLERY survey to quantify the amount of low-mass dark matter haloes within the lensing galaxies and along their lines of sight, and to constrain the properties of dark…

宇宙学与河外天体物理 · 物理学 2019-02-20 E. Ritondale , S. Vegetti , G. Despali , M. W. Auger , L. V. E Koopmans , J. P. McKean

We study the stellar haloes of galaxies out to 70-100 kpc as a function of stellar mass and galaxy type by stacking aligned $r$ and $g$ band images from a sample of 45508 galaxies from SDSS DR9 in the redshift range $0.06\,\le\,z\,\le\,0.1$…

星系天体物理 · 物理学 2015-06-19 R. D'Souza , G. Kauffmann , J. Wang , S. Vegetti

The results of the stellar photometry of the images ACS/WFC and WFPC2 of the HST are used to study stellar population and spatial distribution of stars in three edge-on galaxies: NGC 891, NGC 4144 and NGC 4244. The measuring of the number…

天体物理学 · 物理学 2009-11-10 N. A. Tikhonov , O. A. Galazutdinova

We investigate the globular cluster system around the low-luminosity S0 galaxy NGC 7457 with deep B, V, I photometry. From the V photometry the total number of globular clusters around the galaxy is estimated to be 178 +- 75. The specific…

天体物理学 · 物理学 2007-05-23 S. Chapelon , V. Buat , D. Burgarella , M. Kissler-Patig

We report on the detection of a stellar halo around NGC 1560, a 10^9 Mo spiral galaxy member of the Maffei group. We obtained deep images in the r and i bands using the 10.4m Gran Telescopio Canarias in a field centered at ~ 3.7 arcmin…

星系天体物理 · 物理学 2018-07-25 Laura Greggio , Renato Falomo , Riccardo Scarpa

We obtained very deep exposures of NGC 5907 with a Schmidt telescope, large-format CCD, and intermediate-band filters centered at 6660A and 8020A. These two filters, part of a 15-filter set, are custom-designed to avoid the brightest (and…

天体物理学 · 物理学 2007-05-23 BATC Collaboration , Z. Y. Zheng , Z. H. Shang , H. J. Su , D. Burstein , J. S. Chen

We study the faint stellar halo of isolated central galaxies, by stacking galaxy images in the HSC survey and accounting for the residual sky background sampled with random points. The surface brightness profiles in HSC $r$-band are…

Stellar halos of galaxies, primarily formed through the accretion of smaller objects, are important to understand the hierarchical mass assembly of galaxies. However, the inner regions of stellar halos in disk galaxies are predicted to have…

The faint stellar halos of galaxies contain key information about the oldest stars and the process of galaxy formation. A previous study of stacked SDSS images of disk galaxies has revealed a halo with an abnormally red r-i colour,…

宇宙学与河外天体物理 · 物理学 2015-05-14 Nils Bergvall , Erik Zackrisson , Brady Caldwell

We present the resolved stellar populations in the inner and outer halo of the nearby lenticular galaxy NGC~3115. Using deep HST observations, we analyze stars two magnitudes fainter than the tip of the red giant branch (TRGB). We study…

星系天体物理 · 物理学 2015-06-23 Mark B. Peacock , Jay Strader , Aaron J. Romanowsky , Jean P. Brodie

Various theoretical models predict the existence of extended $\gamma$-ray halo around normal galaxies that could be produced by interactions of cosmic rays with the circumgalactic medium or by annihilation or decay of hypothetical dark…

高能天体物理现象 · 物理学 2026-04-03 M. S. Pshirkov , B. A. Nizamov

We characterize the spatial density of the Pan-STARRS1 (PS1) sample of RR Lyrae stars, to study the properties of the old Galactic stellar halo as traced by RRab stars. This sample of 44,403 sources spans Galactocentric radii of $0.55 \;…

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