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相关论文: Stellar Populations in the Andromeda V Dwarf Spher…

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We present images and a color-magnitude diagram for And V, a new dwarf spheroidal companion to M31 that was found using a digital filtering technique applied to 1550 square degrees of the second Palomar Sky Survey. And V resolves into stars…

天体物理学 · 物理学 2009-10-30 Taft E. Armandroff , James E. Davies , George H. Jacoby

We present B,V time-series photometry of Andromeda XIX (And XIX), the most extended (half-light radius of 6.2') of Andromeda's dwarf spheroidal companions, that we observed with the Large Binocular Cameras at the Large Binocular Telescope.…

B and V time-series photometry of the M31 dwarf spheroidal satellite Andromeda XXI (And XXI) was obtained with the Large Binocular Cameras at the Large Binocular Telescope. We have identified 50 variables in And XXI, of which 41 are RR…

星系天体物理 · 物理学 2015-05-15 F. Cusano , A. Garofalo , G. Clementini , M. Cignoni , L. Federici , M. Marconi , I. Musella , V. Ripepi , R. Speziali , E. Sani , R. Merighi

The Hubble Space Telescope WFPC2 camera has been used to image Andromeda III, a dwarf spheroidal companion (dSph) to M31. The resulting color-magnitude (c-m) diagrams reveal the morphology of the horizontal branch (HB) in this dwarf galaxy.…

天体物理学 · 物理学 2009-11-07 G. S. Da Costa , T. E. Armandroff , Nelson Caldwell

We present B and V time-series photometry of Andromeda XXV, the third galaxy in our program on the Andromeda's satellites, that we have imaged with the Large Binocular Cameras of the Large Binocular Telescope. The field of Andromeda XXV is…

We present B and V time series photometry of the M31 satellite galaxy Andromeda XXVII (And XXVII) that we observed with the Large Binocular Cameras of the Large Binocular Telescope. In the field of And XXVII we have discovered a total of 90…

The HST WFPC2 camera has been used to image Andromeda II, a dwarf spheroidal (dSph) companion to M31. The resulting color-magnitude diagrams reveal the morphology of the horizontal branch (HB) in this dwarf galaxy. We find that like…

天体物理学 · 物理学 2009-10-31 G. S. Da Costa , T. E. Armandroff , Nelson Caldwell , Patrick Seitzer

HST-WFPC2 F555W and F814W photometry were obtained for 16 fields of the luminous nearby spiral galaxy M31, sampling the stellar content of the disk and the halo at different distances from the center, from ~ 20 to ~ 150 arcmin (i.e. ~ 4.5…

天体物理学 · 物理学 2011-07-18 M. Bellazzini , C. Cacciari , L. Federici , F. Fusi Pecci , R. M. Rich

We have surveyed Andromeda VI, a dwarf spheroidal galaxy companion to M31, for variable stars using F450W and F555W observations obtained with the Hubble Space Telescope. A total of 118 variables were found, with 111 being RR Lyrae, 6…

天体物理学 · 物理学 2009-11-07 Barton J. Pritzl , Taft E. Armandroff , George H. Jacoby , Gary S. Da Costa

We have obtained spectra for 50 candidate red giants in Andromeda II (a dwarf spheroidal companion of M31) using LRIS on the Keck II telescope. After eliminating background galaxies and Galactic foreground stars, we are left with a sample…

天体物理学 · 物理学 2009-10-31 Patrick Cote , J. B. Oke , Judith G. Cohen

(abridged) We present the results of a variable star search in Andromeda II, a dwarf spheroidal galaxy companion to M31, using HST/WFPC2 observations. Seventy-three variables were found, one of which is an anomalous Cepheid while the others…

天体物理学 · 物理学 2009-11-10 Barton J. Pritzl , Taft E. Armandroff , George H. Jacoby , G. S. Da Costa

g', r', and i' images obtained with the Gemini Multi-Object Spectrograph (GMOS) on Gemini North are used to investigate the metallicity and stellar content of the M31 dwarf spheroidal companion galaxy And V. Red giant branch (RGB) stars are…

天体物理学 · 物理学 2007-05-23 T. J. Davidge , G. S. Da Costa , I. Jorgensen , J. R. Allington-Smith

We present spectroscopic observations of red giant branch (RGB) stars over a large expanse in the halo of the Andromeda spiral galaxy (M31), acquired with the DEIMOS instrument on the Keck II 10-m telescope. Using a combination of five…

(Abridged) We present the results of variable star searches of the M31 dwarf spheroidal companions Andromeda I and Andromeda III using the Hubble Space Telescope. A total of 100 variable stars were found in Andromeda I, while 56 were found…

天体物理学 · 物理学 2009-11-10 Barton J. Pritzl , Taft E. Armandroff , George H. Jacoby , G. S. Da Costa

A rich harvest of RR Lyrae stars has been identified for the first time in B514, a metal-poor ([Fe/H] = 1.95 +/- 0.10 dex) globular cluster of the Andromeda galaxy (M31), based on Hubble Space Telescope Wide Field Planetary Camera 2 and…

We present a study of the stellar populations in two faint M31 dwarf satellites, Andromeda XI and Andromeda XIII. Using archival images from the Wide Field Planetary Camera 2 (WFPC2) onboard the Hubble Space Telescope (HST), we characterize…

星系天体物理 · 物理学 2015-05-30 Soung-Chul Yang , Ata Sarajedini

We present HST/ACS observations of RR Lyrae variable stars in six ultra deep fields of the Andromeda galaxy (M31), including parts of the halo, disk, and giant stellar stream. Past work on the RR Lyrae stars in M31 has focused on various…

Images have been obtained with the Hubble Space Telescope WFPC2 camera of Andromeda I, a dwarf spheroidal (dSph) galaxy that lies in the outer halo of M31. The resulting color-magnitude diagrams reveal for the first time the morphology of…

天体物理学 · 物理学 2009-10-28 G. S. Da Costa , T. E. Armandroff , Nelson Caldwell , Patrick Seitzer

Photometry in B, V (down to V ~ 26 mag) is presented for two 23' x 23' fields of the Andromeda galaxy (M31) that were observed with the blue channel camera of the Large Binocular Telescope during the Science Demonstration Time. Each field…

We use deep wide-field photometry from the Large Binocular Camera to study the stellar and structural properties of the recently discovered Andromeda X and Andromeda XVII (And X and And XVII) dwarf galaxies. Using the mean apparent…

宇宙学与河外天体物理 · 物理学 2015-05-27 Crystal Brasseur , Hans-Walter Rix , Nicolas F. Martin , Mike Irwin , Annette M. Ferguson , Alan W. McConnachie , Jelte de Jong
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