965 research outputs found
Swift/UVOT Photometry of the Planetary Nebula WeBo 1: Unmasking A Faint Hot Companion Star
We present an analysis of over 150 ks of data on the planetary nebula WeBo 1
(PN G135.6+01.0) obtained with the Swift Ultraviolet Optical Telescope (UVOT).
The central object of this nebula has previously been described as a late-type
K giant barium star with a possible hot companion, most likely a young
pre-white dwarf. UVOT photometry shows that while the optical photometry is
consistent with a large cool object, the near-ultraviolet (UV) photometry shows
far more UV flux than could be produced by any late-type object. Using model
stellar atmospheres and a comparison to UVOT photometry for the pre-white dwarf
PG 1159-035, we find that the companion has a temperature of at least 40,000 K
and a radius of, at most, 0.056 R_sun. While the temperature and radius are
consistent with a hot compact stellar remnant, they are lower and larger,
respectively, than expected for a typical young pre-white dwarf. This likely
indicates a deficiency in the assumed UV extinction curve. We find that higher
temperatures more consistent with expectations for a pre-white dwarf can be
derived if the foreground dust has a strong "blue bump" at 2175 AA and a lower
R_V. Our results demonstrate the ability of Swift to both uncover and
characterize hot hidden companion stars and to constrain the UV extinction
properties of foreground dust based solely on UVOT photometry.Comment: 26 pages, 9 figure, accepted to Astronomical Journa
The uBVI Photometric System. II. Standard Stars
Paper I of this series described the design of a CCD-based photometric system
that is optimized for ground-based measurements of the size of the Balmer
discontinuity in stellar spectra. This "uBVI" system combines the Thuan-Gunn u
filter with the standard Johnson-Kron-Cousins BVI filters, and it can be used
to discover luminous yellow supergiants in extragalactic systems and
post-asymptotic-giant-branch stars in globular clusters and galactic halos. In
the present paper we use uBVI observations obtained on 54 nights with 0.9-m
telescopes at Kitt Peak and Cerro Tololo to construct a catalog of standardized
u magnitudes for standard stars taken from the 1992 catalog of Landolt. We
describe the selection of our 14 Landolt fields, and give details of the
photometric reductions, including red-leak and extinction corrections,
transformation of all of the observations onto a common magnitude system, and
establishment of the photometric zero point. We present a catalog of u
magnitudes of 103 stars suitable for use as standards. We show that data
obtained with other telescopes can be transformed to our standard system with
better than 1% accuracy.Comment: 24 pages, 4 figures, 4 tables; accepted by A
Critical conditions for the wetting of soils
The wettability of soil is of great importance for plants and soil biota and in determining whether flooding and soil erosion will occur. The analysis used in common measurements of soil hydrophobicity makes the assumption that water always enters soils if the average contact angle between the soil and water is 90 degrees or lower; these tests have been used for decades. The authors show theoretically and experimentally that water cannot enter many soils unless the contact angle is considerably lower than this, down to approximately 50 degrees. This difference generates serious errors in determining and modeling soil wetting behavior
La boîte à outils géotechniques de demain: EN 1997-1: 202x Règles générales
This paper describes the development of the final Project Team (PT) draft of the next generation
of Eurocode 7 Part 1 (EN 1997-1:202x). The use of Nationally Determined Parameters and the drive for ease-of-use is highlighted. Key changes from the previous version of EN 1997-1 are explained, including the introduction of the Geotechnical Design Model; revision of the Geotechnical Categories and their application; the implementation of Consequence Classes and Geotechnical Complexity Classes in achieving the reliability required by the Eurocodes; elaboration on the use of numerical methods within Eurocode 7; the treatment of rock on an equal basis with soil; and greater emphasis on the Observational Method.Postprint (published version
The Inflation-Hedging Effectiveness of Real Estate
Inflation has become one of the predominant financial concerns of the late twentieth century. In the late 1970s, public opinion polls ranked inflation as the number one problem in the United States. While the rate of inflation has slowed since the late 1970s, inflation is still present and many investors expect a resurgence of inflation to higher levels in the near to immediate future. This continued concern about inflation has led to an increased search and evaluation of investments that will protect investors from inflation. Assets that have the ability to protect investors from the effects of inflation are generally labeled inflation hedges. Real estate has been regarded as one of the best inflation hedges of past years. While there has been research in the past evaluating this possibility and some recent research using only business real estate, no current research on residential real estate or farmland as inflation hedges exists. This study examines the inflation-hedging effectiveness of residential real estate, farmland, and business real estate (with a different data set) as individual assets and in a portfolio context for 1960-86.
Light-Element Abundance Variations at Low Metallicity: the Globular Cluster NGC 5466
We present low-resolution (R~850) spectra for 67 asymptotic giant branch
(AGB), horizontal branch and red giant branch (RGB) stars in the
low-metallicity globular cluster NGC 5466, taken with the VIRUS-P
integral-field spectrograph at the 2.7-m Harlan J. Smith telescope at McDonald
Observatory. Sixty-six stars are confirmed, and one rejected, as cluster
members based on radial velocity, which we measure to an accuracy of 16 km s-1
via template-matching techniques. CN and CH band strengths have been measured
for 29 RGB and AGB stars in NGC 5466, and the band strength indices measured
from VIRUS-P data show close agreement with those measured from Keck/LRIS
spectra previously taken of five of our target stars. We also determine carbon
abundances from comparisons with synthetic spectra. The RGB stars in our data
set cover a range in absolute V magnitude from +2 to -3, which permits us to
study the rate of carbon depletion on the giant branch as well as the point of
its onset. The data show a clear decline in carbon abundance with rising
luminosity above the luminosity function "bump" on the giant branch, and also a
subdued range in CN band strength, suggesting ongoing internal mixing in
individual stars but minor or no primordial star-to-star variation in
light-element abundances.Comment: 10 pages, emulateapj format, AJ accepte
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