1,531 research outputs found
Cyclical Flow: Spatial Synthesis Sound Toy as Multichannel Composition Tool
This paper outlines and discusses an interactive system designed as a playful âsound toyâ for spatial composition. Proposed models of composition and design in this context are discussed. The design, functionality and application of the software system is then outlined and summarised. The paper concludes with observations from use, and discussion of future developments
The Star Formation Histories of Two Northern LMC Fields
Ground-based UBV photometry of two fields in the northern disk of the LMC are
presented. A distance modulus of (m-M)_0 = 18.41 +/- 0.04 and an extinction of
A_V = 0.30 +/- 0.05 has been calculated for these fields. The measurable star
formation history of the LMC began no more than 12 Gyr ago with a strong star
forming episode with [Fe/H] = -1.63 +/- 0.10 that accounted for approximately
half (by mass) of the LMC's total star formation in the first 3 Gyr. The data
does not give accurate star formation rates during intermediate ages, but there
appears to have been a recent increase in the star formation rate in these
fields, beginning approximately 2.5 Gyr ago, with the current metallicity in
the region being [Fe/H] = -0.38 +/- 0.10. The two fields have had very similar
star formation rates until 200 Myr ago, at which point one shows a large
increase.Comment: 8 pages, 11 figures Accepted for publication in MNRA
The Star-Forming Region NGC 346 in the Small Magellanic Cloud with Hubble Space Telescope ACS Observations I. Photometry
We present a photometric study of the star-forming region NGC 346 and its
surrounding field in the Small Magellanic Cloud, using data taken with the
Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST).
The data set contains both short and long exposures for increased dynamic
range, and photometry was performed using the ACS module of the stellar
photometry package DOLPHOT. We detected almost 100,000 stars over a magnitude
range of V ~ 11 to V ~ 28 mag, including all stellar types from the most
massive young stars to faint lower main sequence and pre-main sequence stars.
We find that this region, which is characterized by a plethora of stellar
systems and interesting objects, is an outstanding example of mixed stellar
populations. We take into account different features of the color-magnitude
diagram of all the detected stars to distinguish the two dominant stellar
systems: The stellar association NGC 346 and the old spherical star cluster BS
90. These observations provide a complete stellar sample of a field about 5
arcmin x 5 arcmin around the most active star-forming region in this galaxy.
Considering the importance of these data for various investigations in the
area, we provide the full stellar catalog from our photometry. This paper is
the first part of an ongoing study to investigate in detail the two dominant
stellar systems in the area and their surrounding field.Comment: 8 pages, 5 figures, Accepted for publication in The Astrophysical
Journal Supplement Series, A high-resolution version can be found at:
http://www.astro.uni-bonn.de/~dgoulier/Science/Gouliermis+_NGC346_I.pd
Calibration of BVRI Photometry for the Wide Field Channel of the HST Advanced Camera for Surveys
We present new observations of two Galactic globular clusters, PAL4 and
PAL14, using the Wide-Field Channel of the Advanced Camera for Surveys (ACS) on
board the Hubble Space Telescope (HST), and reanalyze archival data from a
third, NGC2419. We matched our photometry of hundreds of stars in these fields
from the ACS images to existing, ground-based photometry of faint sequences
which were calibrated on the standard BVRI system of Landolt. These stars are
significantly fainter than those generally used for HST calibration purposes,
and therefore are much better matched to supporting precision photometry of ACS
science targets. We were able to derive more accurate photometric
transformation coefficients for the commonly used ACS broad-band filters
compared to those published by Sirianni, et al. (2005), owing to the use of a
factor of several more calibration stars which span a greater range of color.
We find that the inferred transformations from each cluster individually do not
vary significantly from the average, except for a small offset of the
photometric zeropoint in the F850LP filter. Our results suggest that the
published prescriptions for the time-dependent correction of CCD
charge-transfer efficiency appear to work very well over the ~3.5 yr interval
that spans our observations of PAL4 and PAL14 and the archived images of
NGC2419.Comment: 22 pages, 12 figures. Accepted for publication in PAS
HST Survey of Clusters in Nearby Galaxies. II. Statistical Analysis of Cluster Populations
We present a statistical system that can be used in the study of cluster
populations. The basis of our approach is the construction of synthetic cluster
color-magnitude-radius diagrams (CMRDs), which we compare with the observed
data using a maximum likelihood calculation. This approach permits a relatively
easy incorporation of incompleteness (a function of not only magnitude and
color, but also radius), photometry errors and biases, and a variety of other
complex effects into the calculation, instead of the more common procedure of
attempting to correct for those effects.
We then apply this procedure to our NGC 3627 data from Paper I. We find that
we are able to successfully model the observed CMRD and constrain a number of
parameters of the cluster population. We measure a power law mass function
slope of alpha = -1.50 +/- 0.07, and a distribution of core radii centered at
r_c = 1.53 +/- 0.15 pc. Although the extinction distribution is less
constrained, we measured a value for the mean extinction consistent with that
determined in Paper I from the Cepheids.Comment: 21 pages, 3 figures accepted for publication by A
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