6,705 research outputs found
Exploring the reality of density substructures in the Palomar 5 stellar stream
We present an analysis of the presence of substructures in the stellar stream
of the Palomar 5 globular cluster, as derived from Sloan Digital Sky Survey
data. Using a matched filter technique, we recover the positions and sizes of
overdensities reported in previous studies. To explore the reality of these
structures, we also create an artificial model of the stream, in which we
construct a realistic background on top of which we add a perfectly smooth
stream structure, taking into account the effects of photometric completeness
and interstellar extinction. We find that the smooth artificial stream then
shows similarly-pronounced substructures as the real structure. Interestingly,
our best-fit N-body simulation does display real projected density variations
linked to stellar epicyclic motions, but these become less significant when
taking into account the SDSS star-count constraints. The substructures found
when applying our matched filter technique to the N-body particles converted
into observable stars are thus mostly unrelated to these epicyclic motions.
This analysis suggests that the majority of the previously-detected
substructures along the tidal tail of Palomar 5 are artefacts of observational
inhomogeneities.Comment: 10 pages, 9 figures, accepted for publication in MNRA
Galactic halo stellar structures in the Triangulum-Andromeda region
This letter reports on the Galactic stellar structures that appear in the
foreground of our Canada-France-Hawaii-Telecopse/MegaCam survey of the halo of
the Andromeda galaxy. We recover the main sequence and main sequence turn-off
of the Triangulum-Andromeda structure recently found by Majewski and
collaborators at a heliocentric distance of ~20 kpc. The survey also reveals
another less populated main sequence at fainter magnitudes that could
correspond to a more distant stellar structure at ~28 kpc. Both structures are
smoothly distributed over the ~76 sq. deg. covered by the survey although the
closer one shows an increase in density by a factor of ~2 towards the
North-West. The discovery of a stellar structure behind the
Triangulum-Andromeda structure that itself appears behind the low-latitude
stream that surrounds the Galactic disk gives further evidence that the inner
halo of the Milky Way is of a spatially clumpy nature.Comment: accepted for publication in ApJL, 4 pages, 4 figures. Significant
changes including a larger dataset and a more thorough discussio
The Canis Major Dwarf Galaxy
Recent observational evidence suggests that the Sagittarius dwarf galaxy
represents the only major ongoing accretion event in the Galactic halo,
accounting for the majority of stellar debris identified there. This paper
summarizes the recent discovery of another potential Milky Way accretion event,
the Canis Major dwarf galaxy. This dwarf satellite galaxy is found to lie just
below the Galactic plane and appears to be on an equatorial orbit. Unlike
Sagittarius, which is contributing to the Galactic halo, the location and
eventual demise of Canis Major suggests that it represents a building block of
the thick disk.Comment: Refereed contribution to "Structure & Dynamics in the Local Universe,
a workshop to honour Brent Tully's 60th birthday", Nov 2003. 4 pages + 2
figures (quality reduced due to size restrictions). To appear in PAS
Correcting the influence of an asymmetric line spread function in 2-degree Field spectrograph data
We investigate the role of asymmetries in the line spread function of the
2-degree field spectrograph and the variations in these asymmetries with the
CCD, the plate, the time of observation and the fibre. A data-reduction
pipeline is developed that takes these deformations into account for the
calibration and cross-correlation of the spectra. We show that, using the
emission lines of calibration lamp observations, we can fit the line spread
function with the sum of two Gaussian functions representing the theoretical
signal and a perturbation of the system. This model is then used to calibrate
the spectra and generate templates by downgrading high resolution spectra.
Thus, we can cross-correlate the observed spectra with templates degraded in
the same way. Our reduction pipeline is tested on real observations and
provides a significant improvement in the accuracy of the radial velocities
obtained. In particular, the systematic errors that were as high as ~20 km/s
when applying the AAO reduction package 2dfDR are now reduced to ~5 km/s. Even
though the 2-degree Field spectrograph is to be decommissioned at the end of
2005, the analysis of archival data and previous studies could be improved by
the reduction procedure we propose here.Comment: 9 pages, 9 figures, accepted to PASA, minor change
Andromeda XXIX: A New Dwarf Spheroidal Galaxy 200Â kpc from Andromeda
We report the discovery of a new dwarf galaxy, Andromeda XXIX (And XXIX), using data from the recently released Sloan Digital Sky Survey Data Release 8, and confirmed by Gemini North telescope Multi-Object Spectrograph imaging data. And XXIX appears to be a dwarf spheroidal galaxy, separated on the sky by a little more than 15° from M31, with a distance inferred from the tip of the red giant branch of 730 ± 75 kpc, corresponding to a three-dimensional separation from M31 of 207 +20 – 2 kpc (close to M31's virial radius). Its absolute magnitude, as determined by comparison to the red giant branch luminosity function of the Draco dwarf spheroidal, is M V = –8.3 ± 0.4. And XXIX's stellar populations appear very similar to Draco's; consequently, we estimate a metallicity for And XXIX of [Fe/H] ~–1.8. The half-light radius of And XXIX is 360 ± 60 pc and its ellipticity is 0.35 ± 0.06, typical of dwarf satellites of the Milky Way and M31 at this absolute magnitude range.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/90744/1/2041-8205_742_1_L15.pd
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