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相关论文: A Survey for Low Surface Brightness Dwarf Galaxies…

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Using Virtual Observatory tools, we cross-matched the Carlsberg Meridian 14 and the 2MASS Point Source catalogs to select candidate nearby bright M dwarfs distributed over ~ 25,000 deg^2. Here, we present reconnaissance low-resolution…

太阳与恒星天体物理 · 物理学 2014-09-17 M. Aberasturi , J. A. Caballero , B. Montesinos , M. C. Gálvez-Ortiz , E. Solano , E. L. Martín

An all-sky list of 88 nearby dwarf spheroidal (dSph) galaxies with distances D < 10 Mpc is considered. Most of the objects have recently been found by Karachentseva & Karachentsev based on POSSII/ESO-SERC survey. A hundred more dSph…

天体物理学 · 物理学 2009-11-11 I. D. Karachentsev , V. E. Karachentseva , M. E. Sharina

We undertook a search for new nearby dwarf galaxies outside the known groups in the Local Volume using the data on DESI Legacy Imaging Surveys. In a wide sky area of $\sim$5000 square degrees directed toward the Local Void, we found only 12…

星系天体物理 · 物理学 2023-12-11 I. D. Karachentsev , V. E. Karachentseva , S. S. Kaisin , E. I. Kaisina

We obtained follow-up HST observations of the seven low surface brightness galaxies discovered with the Dragonfly Telephoto Array in the field of the massive spiral galaxy M101. Out of the seven galaxies, only three were resolved into stars…

We present surface photometry and metallicity measurements for 104 nearby dwarf galaxies imaged with the Advanced Camera for Surveys and Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope. In addition, we carried out…

We survey a sample of 32 M5-M8 stars with distance < 40pc for companions with separations between 0.1 arcsec and 1.5 arcsec and with Delta m_i <5. We find five new VLM binaries with separations between 0.15 arcsec and 1.1 arcsec, including…

天体物理学 · 物理学 2009-11-11 N. M. Law , S. T. Hodgkin , C. D. Mackay

We present optical long-slit spectroscopy and far-ultraviolet to near-infrared spectral energy distribution fitting of two diffuse dwarf galaxies, LSBG-285 and LSBG-750, which were recently discovered by the Hyper Suprime-Cam Subaru…

We report the discovery of 11 newly found quasars behind the stellar disks of the spiral galaxies M31 and M33 in the fields covered by the Local Group Galaxy Survey. Their redshifts range from 0.37 to 2.15. Most are X-ray, UV, and IR…

星系天体物理 · 物理学 2020-01-08 Philip Massey , Kathryn F. Neugent , Emily M. Levesque

We report observations of five dwarf galaxies in the vicinity of the luminous S0 galaxy NGC 3115 performed with the Advanced Camera for Surveys on the Hubble Space Telescope. Their distances determined via the Tip of the Red Giant Branch…

星系天体物理 · 物理学 2022-05-04 I. D. Karachentsev , L. N. Makarova , G. S. Anand , R. B. Tully

The nature of the dwarf galaxy population as a function of location in the cluster and within different environments is investigated. We have previously described the results of a search for low surface brightness objects in data drawn from…

天体物理学 · 物理学 2009-11-13 S. Sabatini , J. I. Davies , S. Roberts , R. Scaramella

We present results from a spectroscopic survey of the dwarf spheroidal And XXII and the two extended clusters EC1 and EC2. These three objects are candidate satellites of the Triangulum galaxy, M33, which itself is likely a satellite of…

We obtained B and R-band CCD images for the dwarf elliptical (dE) galaxies DDO44, UGC4998, KK98_77, DDO71, DDO113, and UGC7356 at the NOT. Using Fourier analysis technique we measure stellar R-band surface brightness fluctuations (SBFs) and…

天体物理学 · 物理学 2009-11-07 Helmut Jerjen , Rami Rekola , Leo Takalo , Matthew Coleman , Mauri Valtonen

We present a photometric study of the Andromeda XVIII dwarf spheroidal galaxy associated with M31, and situated well outside of the virial radius of the M31 halo. The galaxy was resolved into stars with Hubble Space Telescope/Advanced…

星系天体物理 · 物理学 2016-10-12 L. N. Makarova , D. I. Makarov , I. D. Karachentsev , R. B. Tully , L. Rizzi

We report the discovery of twenty-one hitherto unknown bright southern ultracool dwarfs with spectral types in the range M7 to L5.5, together with new observations of a further three late M dwarfs previously confirmed. Three more objects…

We present the results of an all-sky, deep optical survey for faint Local Group dwarf galaxies. Candidate objects were selected from the second Palomar survey (POSS-II) and ESO/SRC survey plates and follow-up observations performed to…

天体物理学 · 物理学 2008-11-26 Alan B. Whiting , George K. T. Hau , Mike Irwin , Miguel Verdugo

We present spectra of 59 nearby stars candidates, M dwarfs and white dwarfs, previously identified using high proper motion catalogues and the DENIS database. We review the existing spectral classification schemes and spectroscopic parallax…

天体物理学 · 物理学 2009-11-11 C. Reyle , R. -D. Scholz , M. Schultheis , A. C. Robin , M. Irwin

We present a study of the smallest and faintest galaxies found in a very deep photographic R band survey of two regions of the Virgo Cluster, totalling 3.2 square degrees, made with the UK Schmidt Telescope. The objects we detect have the…

天体物理学 · 物理学 2009-09-25 J. B. Jones , S. Phillipps , J. M. Schwartzenberg , Q. A. Parker

We report the first results from deep ACS imaging of ten classical globular clusters in the far outer regions (15 < R_p < 100 kpc) of M31. Eight of the clusters, including two of the most remote M31 globular clusters presently known, are…

天体物理学 · 物理学 2009-11-11 A. D. Mackey , A. Huxor , A. M. N. Ferguson , N. R. Tanvir , M. Irwin , R. Ibata , T. Bridges , R. A. Johnson , G. Lewis

We have created 0.3--10 keV, 13 year, unabsorbed luminosity lightcurves for 528 X-ray sources in the central 20' of M31. We have 174 Chandra observations spaced at ~1 month intervals thanks to our transient monitoring program, deeper…

高能天体物理现象 · 物理学 2015-06-17 R. Barnard , M. R. Garcia , F. Primini , Z. Li , F. Baganoff , S. S. Murray

We have previously presented the results of a 325 MHz radio survey of M31, conducted with the A-configuration of the Very Large Array. In this survey, a total of 405 radio sources between <6" and 170" in extent were mapped with a resolution…

天体物理学 · 物理学 2009-11-11 Joseph D. Gelfand , T. J. W. Lazio , B. M. Gaensler