2,705 research outputs found
A report of the physiological, psychological, and bacteriological aspects of 20 days in full pressure suits, 20 days at 27,000 feet on 100 per cent oxygen, and 34 days of confinement, part III Final report, 2 Jun. 1964 - Nov. 1965
Physiological, psychological, and bacteriological aspects of 20 days in full pressure suits, 20 days at 27.000 feet on 100 percent oxygen, and 34 days of confinemen
A computer operated mass spectrometer system
Digital computer system for processing mass spectrometer output dat
Discovery of a flux-related change of the cyclotron line energy in Her X-1
We present the results of ten years of repeated measurements of the Cyclotron
Resonance Scattering Feature (CRSF) in the spectrum of the binary X-ray pulsar
Her X-1 and report the discovery of a positive correlation of the centroid
energy of this absorption feature in pulse phase averaged spectra with source
luminosity.Our results are based on a uniform analysis of observations bythe
RXTE satellite from 1996 to 2005, using sufficiently long observations of 12
individual 35-day Main-On states of the source. The mean centroid energy E_c of
the CRSF in pulse phase averaged spectra of Her X-1 during this time is around
40 keV, with significant variations from one Main-On state to the next. We find
that the centroid energy of the CRSF in Her X-1 changes by ~5% in energy for a
factor of 2 in luminosity. The correlation is positive, contrary to what is
observed in some high luminosity transient pulsars. Our finding is the first
significant measurement of a positive correlation between E_c and luminosity in
any X-ray pulsar. We suggest that this behaviour is expected in the case of
sub-Eddington accretion and present a calculation of a quantitative estimate,
which is very consistent with the effect observed in Her X-1.We urge that Her
X-1 is regularly monitored further and that other X-ray pulsars are
investigated for a similar behaviour.Comment: 4 pages, 2 figures, accepted by A&A Letter
Approaches Mainline Protestant Pastors Use to Work with LGB People and Their Families: Implications for Family Therapists
When a loved one comes out as lesbian, gay, or bisexual (LGB), families often seek the assistance of a trusted professional. For many families that involves seeking the consultation of a religious leader. This queer theory informed qualitative study sought to explore how Christian pastors work with LGB individuals and their families. Additionally, this study explored how pastors’ approaches to working with LGB individuals and their families varied based on the degree to which families were accepting or rejecting of their LGB family members. Twenty-one mainline Protestant Christian pastors were interviewed. Thematic analysis identified three themes and a number of subthemes that provide new insights for family therapists by highlighting that pastors engaged in theological conversations with families to encourage acceptance, walked with families in their journey of navigating external discrimination, and provided resources such as connection to community services and referrals to family therapy
Multiple Cyclotron Lines in the Spectrum of 4U 0115+63
We report phase resolved spectroscopy of the transient accreting pulsar,
4U0115+63. For the first time, more than two cylotron resonance scattering
features are detected in the spectrum of an X-ray pulsar. The shape of the
fundamental line appears to be complex, and this is in agreement with
predictions of Monte-Carlo models. As in other pulsars, the line energies and
optical depths are strong functions of pulse phase. One possible model for this
is an offset of the dipole of the neutron star magnetic field.Comment: 5 pages. To appear in "Proceedings of the 5th Compton Symposium
INTEGRAL observations of V0332+53 in outburst
We present the analysis of a 100ksec Integral(3-100kev) observation of the
transient X-ray pulsar V0332+53 inoutburst. The source is pulsating at
P=4.3751+/-0.0002s with a clear double pulse from 6 kev to 60 kev. The average
flux was ~550mCrab between 20 kev and 60 kev. We modeled the broad band
continuum from 5 kev to 100 kev with a power-law modified by an exponential cut
off. We observe three cyclotron lines: the fundamental line at 24.9+/-0.1 kev,
the first harmonic at 50.5+/-0.1 kev as well as the second harmonic
at71.7+/-0.8 kev, thus confirming the discovery of the harmonic lines by Coburn
et al. (2005) in RXTE data.Comment: 4 pages, 3 figures. Accepted for publication in A&A Letter
Discovery of a Cyclotron Resonance Scattering Feature in the X-ray Spectrum of XTE J1946+274
Observations of the transient accreting pulsar XTE J1946+274 made with the
Rossi X-ray Timing Explorer during the course of the 1998 September-November
outburst, reveal a cyclotron resonance scattering feature (or "cyclotron line")
in the hard X-ray spectrum near 35 keV. We determine a centroid energy of 36.2
+0.5/-0.7 keV, which implies a magnetic field strength of 3.1(1+z)x10^12 G,
where z is the gravitational redshift of the scattering region. The optical
depth, Tau = 0.33 +0.07/-0.06, and width, sigma = 3.37 +0.92/-0.75 keV, are
typical of known cyclotron lines in other pulsars. This discovery makes XTE
J1946+274 one of thirteen pulsars with securely detected cyclotron lines
resulting in direct magnetic field measurements.Comment: Five pages including four postscript figures and two tables. Uses
emulateapj5. Published in ApJ Letters:
http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2001ApJ...563L..35
Gamma-Ray Polarimetry of Two X-Class Solar Flares
We have performed the first polarimetry of solar flare emission at gamma-ray
energies (0.2-1 MeV). These observations were performed with the Reuven Ramaty
High Energy Solar Spectroscopic Imager (RHESSI) for two large flares: the GOES
X4.8-class solar flare of 2002 July 23, and the X17-class flare of 2003 October
28. We have marginal polarization detections in both flares, at levels of 21%
+/- 9% and -11% +/- 5% respectively. These measurements significantly constrain
the levels and directions of solar flare gamma-ray polarization, and begin to
probe the underlying electron distributions.Comment: 33 pages, 12 figures, accepted for publication in Ap
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