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Related papers: Hide and seek between Andromeda's halo, disk, and …

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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…

We present wide and deep photometry of the northwest part of the halo of the Andromeda galaxy (M31) using Hyper Suprime-Cam on the Subaru Telescope. The survey covers 9.2 deg$^{2}$ field in the $g$, $i$, and $NB515$ bands and shows a clear…

(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…

Astrophysics · Physics 2009-11-10 Barton J. Pritzl , Taft E. Armandroff , George H. Jacoby , G. S. Da Costa

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…

Astrophysics of Galaxies · Physics 2017-12-20 F. Cusano , A. Garofalo , G. Clementini , M. Cignoni , T. Muraveva , G. Tessicini , V. Testa , D. Paris , L. Federici , M. Marconi , V. Ripepi , I. Musella

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,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.…

We present a census of variable stars in six M31 dwarf spheroidal satellites observed with the Hubble Space Telescope. We detect 870 RR Lyrae (RRL) stars in the fields of And I (296), II (251), III (111), XV (117), XVI (8), XXVIII (87). We…

We present a spectroscopic survey of the giant stellar stream found in the halo of the Andromeda galaxy. Taken with the DEIMOS multi-object spectrograph on the Keck2 telescope, these data display a narrow velocity dispersion of 11+/-3 km/s,…

Astrophysics · Physics 2009-11-10 R. Ibata , S. Chapman , A. M. N. Ferguson , M. Irwin , G. Lewis , A. McConnachie

We present a statistical characterization of the carbon-star to M-giant (C/M) ratio in the halo of M31. Based on application of pseudo-filter band passes to our Keck/DEIMOS spectra we measure the 81-77-color index of 1288 stars in the giant…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Andreas Koch , R. Michael Rich

Detailed studies of stellar populations in the halos of the Milky Way and the Andromeda (M 31) galaxies have shown increasing numbers of tidal streams and dwarf galaxies, attesting to a complicated and on-going process of hierarchical…

Astrophysics of Galaxies · Physics 2015-07-15 Andreas Koch , Charles W. Danforth , R. Michael Rich , Rodrigo Ibata , Brian A. Keeney

We present evidence for a metal-poor, [Fe/H]$\sim-1.4$ $\sigma$=0.2 dex, stellar halo component detectable at radii from 10 kpc to 70 kpc, in our nearest giant spiral neighbor, the Andromeda galaxy. This metal-poor sample underlies the…

Astrophysics · Physics 2008-11-26 S. C. Chapman , R. Ibata , G. F. Lewis , A. M. N. Ferguson , M. Irwin , A. McConnachie , N. Tanvir

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…

Astrophysics · Physics 2009-11-07 Barton J. Pritzl , Taft E. Armandroff , George H. Jacoby , Gary S. Da Costa

(abridged) We present a spectroscopic analysis of five stellar streams (`A', `B', `Cr', `Cp' and `D') as well as the extended star cluster, EC4, which lies within streamC, all discovered in the halo of M31 from our CFHT/MegaCam survey.…

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…

Astrophysics · Physics 2011-07-18 M. Bellazzini , C. Cacciari , L. Federici , F. Fusi Pecci , R. M. Rich

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…

Astrophysics of Galaxies · Physics 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

(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…

Astrophysics · Physics 2009-11-10 Barton J. Pritzl , Taft E. Armandroff , George H. Jacoby , G. S. Da Costa

The wide-field CCD camera at the CFH telescope was used to survey the giant stellar stream in the Andromeda galaxy, resolving stars down the red giant branch in M31 to I ~ 25, a magnitude deeper than our previous INT survey of this galaxy…

Astrophysics · Physics 2009-11-07 A. W. McConnachie , M. J. Irwin , R. A. Ibata , A. M. N. Ferguson , G. F. Lewis , N. Tanvir

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…

We present the first results from an extended survey of the Andromeda galaxy (M31) using 41.1 h of observations by Spitzer-IRAC at 3.6 and 4.5$\,\mu$m. This survey extends previous observations to the outer disc and halo, covering total…

We characterize the bulge, disk, and halo subcomponents in the Andromeda galaxy (M31) over the radial range 4 < R_proj < 225 kpc. The cospatial nature of these subcomponents renders them difficult to disentangle using surface brightness…

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