215 research outputs found
Astrometric-spectroscopic determination of the absolute masses of the HgMn binary star Phi Herculis
The Mercury-Manganese star Phi Her is a well known spectroscopic binary that
has been the subject of a recent study by Zavala et al. (2006), in which they
resolved the companion using long-baseline interferometry. The total mass of
the binary is now fairly well established, but the combination of the
spectroscopy with the astrometry has not resulted in individual masses
consistent with the spectral types of the components. The motion of the center
of light of Phi Her was clearly detected by the Hipparcos satellite. Here we
make use of the Hipparcos intermediate data (`abscissa residuals') and show
that by combining them in an optimal fashion with the interferometry the
individual masses can be obtained reliably using only astrometry. We re-examine
and then incorporate existing radial-velocity measurements into the orbital
solution, obtaining improved masses of 3.05 +/- 0.24 M_Sun and 1.614 +/- 0.066
M_Sun that are consistent with the theoretical mass-luminosity relation from
recent stellar evolution models. These mass determinations provide important
information for the understanding of the nature of this peculiar class of
stars.Comment: Total of 18 pages including figures and tables, in emulateapj format.
To appear in The Astronomical Journal, June 2007 issu
Effect of Burning on Seedstalk Production of Native Prairie Grasses
This study was conducted on the Hayden prairie, located in northeastern Iowa and involved a further investigation of the effects of burning on the growth of certain native prairie grasses as to relative production of various plant parts. The measurements are of plants taken from an upland prairie area burned in 1956 and an adjacent unburned area
Gender equality and girls education: Investigating frameworks, disjunctures and meanings of quality education
The article draws on qualitative educational research across a diversity of low-income countries to examine the gendered inequalities in education as complex, multi-faceted and situated rather than a series of barriers to be overcome through linear inputâoutput processes focused on isolated dimensions of quality. It argues that frameworks for thinking about educational quality often result in analyses of gender inequalities that are fragmented and incomplete. However, by considering education quality more broadly as a terrain of quality it investigates questions of educational transitions, teacher supply and community participation, and develops understandings of how education is experienced by learners and teachers in their gendered lives and their teaching practices. By taking an approach based on theories of human development the article identifies dynamics of power underpinning gender inequalities in the literature and played out in diverse contexts and influenced by social, cultural and historical contexts. The review and discussion indicate that attaining gender equitable quality education requires recognition and understanding of the ways in which inequalities intersect and interrelate in order to seek out multi-faceted strategies that address not only different dimensions of girlsâ and womenâs lives, but understand gendered relationships and structurally entrenched inequalities between women and men, girls and boys
X-ray Variability in the Young Massive Triple theta2 Ori A
Massive stars rarely show intrinsic X-ray variability. The only O-stars
credited to be intrinsically variable are theta1 Ori C due to effects from
magnetic confinement of its wind, and theta2 Ori A suspected of similar
activity. Early Chandra observations have shown that the most massive star
system in the Orion Trapezium Cluster, theta2 Ori A, shows rapid variability on
time scales of hours. We determine X-ray fluxes and find that the star shows
very strong variability over the last 5 years. We observed a second large X-ray
outburst in November 2004 with the high resolution transmission grating
spectrometer on-board Chandra. In the low state X-ray emissivities indicate
temperatures well above 25 MK. In the high state we find an extended emissivity
distribution with high emissivities in the range from 3 MK to over 100 MK. The
outburst event in stellar terms is one of the most powerful ever observed and
the most energetic one in the ONC with a lower total energy limit of 1.5x10^37
ergs. The line diagnostics show that under the assumption that the line
emitting regions in the low states are as close as within 1 -- 2 stellar radii
from the O-star's photosphere, whereas the hard states suggest a distance of 3
-- 5 stellar radii. The two outbursts are very close to the periastron passage
of the stars. We argue that the high X-ray states are possibly the result of
reconnection events from magnetic interactions of the primary and secondary
stars of the spectroscopic binary. Effects from wind collisions seem unlikely
for this system. The low state emissivity and R-ratios strengthen the
predicament that the X-ray emission is enhanced by magnetic confinement of the
primary wind. We also detect Fe fluorescence indicative of the existence of
substantial amounts of neutral Fe in the vicinity of the X-ray emission.Comment: 11 pages, 8 figures, accepted for publication in The Astrophysical
Main Journa
Indigenous knowledge, skills and action:Indigenous womenâs learning in the Peruvian Amazon
Drawing on long term ethnographic research in the SE Peruvian Amazon this article asks what kinds and forms of learning do indigenous women value, how are the knowledge and skills they value changing over time and what is the nature of their agency in the face of the discrimination and prejudice that permeate their lives. Harakmbut womenâs lives have been transformed over the past 40Â years in the wake of neoliberal globalisation, rapacious exploitative economic practices and unregulated illegal gold mining. Within this context, three types of learning emerge as important: learning about indigenous cosmology and way of life; experiential learning through engagement with an expanding capitalist society; and learning through training and capacity building for participation, voice and rights-based advocacy. The article argues that all three types of learning give meaning to Harakmbut womenâs lives, their relationship to their history and their views of the world
The HgMn Binary Star Phi Herculis: Detection and Properties of the Secondary and Revision of the Elemental Abundances of the Primary
Observations of the Mercury-Manganese star Phi Herculis with the Navy
Prototype Optical Interferometer (NPOI) conclusively reveal the previously
unseen companion in this single-lined binary system. The NPOI data were used to
predict a spectral type of A8V for the secondary star Phi Her B. This
prediction was subsequently confirmed by spectroscopic observations obtained at
the Dominion Astrophysical Observatory. Phi Her B is rotating at 50 +/-3
km/sec, in contrast to the 8 km/sec lines of Phi Her A. Recognizing the lines
from the secondary permits one to separate them from those of the primary. The
abundance analysis of Phi Her A shows an abundance pattern similar to those of
other HgMn stars with Al being very underabundant and Sc, Cr, Mn, Zn, Ga, Sr,
Y, Zr, Ba, Ce, and Hg being very overabundant.Comment: Accepted to ApJ, 45 pages, 11 figure
SN 2009E: a faint clone of SN 1987A
In this paper we investigate the properties of SN 2009E, which exploded in a
relatively nearby spiral galaxy (NGC 4141) and that is probably the faintest
1987A-like supernova discovered so far. Spectroscopic observations which
started about 2 months after the supernova explosion, highlight significant
differences between SN 2009E and the prototypical SN 1987A. Modelling the data
of SN 2009E allows us to constrain the explosion parameters and the properties
of the progenitor star, and compare the inferred estimates with those available
for the similar SNe 1987A and 1998A. The light curve of SN 2009E is less
luminous than that of SN 1987A and the other members of this class, and the
maximum light curve peak is reached at a slightly later epoch than in SN 1987A.
Late-time photometric observations suggest that SN 2009E ejected about 0.04
solar masses of 56Ni, which is the smallest 56Ni mass in our sample of
1987A-like events. Modelling the observations with a radiation hydrodynamics
code, we infer for SN 2009E a kinetic plus thermal energy of about 0.6 foe, an
initial radius of ~7 x 10^12 cm and an ejected mass of ~19 solar masses. The
photospheric spectra show a number of narrow (v~1800 km/s) metal lines, with
unusually strong Ba II lines. The nebular spectrum displays narrow emission
lines of H, Na I, [Ca II] and [O I], with the [O I] feature being relatively
strong compared to the [Ca II] doublet. The overall spectroscopic evolution is
reminiscent of that of the faint 56Ni-poor type II-plateau supernovae. This
suggests that SN 2009E belongs to the low-luminosity, low 56Ni mass, low-energy
tail in the distribution of the 1987A-like objects in the same manner as SN
1997D and similar events represent the faint tail in the distribution of
physical properties for normal type II-plateau supernovae.Comment: 19 pages, 9 figures (+7 in appendix); accepted for publication in A&A
on 3 November 201
A perspective on the measurement of time in plant disease epidemiology
The growth and development of plant pathogens and their hosts generally respond strongly to the temperature of their environment. However, most studies of plant pathology record pathogen/host measurements against physical time (e.g. hours or days) rather than thermal time (e.g. degree-days or degree-hours). This confounds the comparison of epidemiological measurements across experiments and limits the value of the scientific literature
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