1,349 research outputs found
HB 282, Relating to the Establishment of Hawaii Alternate Energy Development Authority - Statement for House Committee Energy, Ecology and Environmental Protection Public Hearing - 20 February 1981
Common Envelope Evolution Leading to Supernovae with Dense Interaction
A variety of supernova events, including Type IIn supernovae and
ultraluminous supernovae, appear to have lost up to solar masses of their
envelopes in 10's to 100's of years leading up to the explosion. In order to
explain the close timing of the mass loss and supernova events, we explore the
possibility that the mass loss is driven by common envelope evolution of a
compact object (neutron star or black hole) in the envelope of a massive star
and the supernova is triggered by the inspiral of the compact object to the
central core of the companion star. The expected rate of such events is smaller
than the observed rate of Type IIn supernovae but the rates may agree within
the uncertainties. The mass loss velocity is related to the escape velocity
from the common envelope system and is comparable to the observed velocity of
100's of km s in Type IIn events. The mass loss is expected to be denser
near the equatorial plane of the binary system and there is good evidence that
the circumstellar media in Type IIn supernovae are asymmetric. Some of these
supernova types show evidence for energies in excess of the canonical
ergs, which might be the result of explosions from rapid accretion onto a
compact object through a disk.Comment: Small changes to agree with published version: ApJ Letters, 752, L2
(2012
In-Depth Global Analysis of Transcript Abundance Levels in Porcine Alveolar Macrophages Following Infection with Porcine Reproductive and Respiratory Syndrome Virus
Porcine reproductive and respiratory syndrome virus (PRRSV) is a major pathogen of swine worldwide and causes considerable economic loss. Identifying specific cell signaling or activation pathways that associate with variation in PRRSV replication and macrophage function may lead to identification of novel gene targets for the control of PRRSV infection. Serial Analysis of Gene Expression (SAGE) was used to create and survey the transcriptome of in vitro mock-infected and PRRSV strain VR-2332-infected porcine alveolar macrophages (PAM) at 0, 6, 12, 16, and 24 hours after infection. The transcriptome data indicated changes in transcript abundance occurring in PRRSV-infected PAMs over time after infection with more than 590 unique tags with significantly altered transcript abundance levels identified (P < .01). Strikingly, innate immune genes (whose transcript abundances are typically altered in response to other pathogens or insults including IL-8, CCL4, and IL-1β) showed no or very little change at any time point following infection
SN2008am: A Super-Luminous Type IIn Supernova
We present observations and interpretation of the Type IIn supernova SN
2008am discovered by the ROTSE Supernova Verification Project (RSVP). SN 2008am
peaked at approximately -22.3 mag at a redshift of z=0.2338, giving it a peak
luminosity of 3 x 10^{44}erg/s and making it one of the most luminous
supernovae ever observed. The total radiated energy is ~ 2 x 10^{51} erg.
Photometric observations in the ultraviolet, optical and infrared bands
(J,H,Ks) constrain the SED evolution. We obtained six optical spectra of the
supernova, five on the early decline from maximum light and a sixth nearly a
year later plus a very late-time spectrum (~2 yr) of the host galaxy. The
spectra of SN 2008am show strong Balmer-line and He I lambda 5876A emission
with intermediate widths (~25A) in the first ~40 days after optical maximum. We
examine a variety of models for the line wings and conclude that multiple
scattering is most likely, implying that our spectra contain no specific
information on the bulk flow velocity. We examine a variety of models for the
ROTSE light curve subject to the rise time and the nature of the spectra,
including radioactive decay, shocks in optically-thick and optically-thin
circumstellar media (CSM) and a magnetar. The most successful model is one for
which the CSM is optically-thick and in which diffusion of forward
shock-deposited luminosity gives rise to the observed light curve. Diffusion of
the shock-deposited energy from the forward shock is found to be important to
account for the rising part of the light curve. Although there are differences
in detail, SN 2008am appears to be closely related to other super-luminous Type
IIn supernovae, SN 2006gy, SN 2006tf and perhaps SN 2008iy, that may represent
the deaths of very massive LBV-type progenitors and for which the luminosity is
powered by the interaction of the ejecta with a dense circumstellar medium.Comment: 58 pages, 14 figure
The Grizzly, October 16, 1981
Long Range Improvements Planned • Homecoming Coming Up • Fraternity Hazing Topic of Next Forum • Sadat: The Champion of Peace • USGA Notes • Procedure and Schedule for Spring Term Registration • Frats Resume Reimert Cleanup • Student Advising Program to be Revised Next Year • Transplanted Texan: Evaluation of a Brown-noser • Increased Internationalism Has Positive Effect on Campus • Bad Weather Attendance Rules • Homecoming Queen Candidates • Community and Civilization Course • Ursinus News Briefs: The law of the sea: is it a new threat to peace?; Exploring career options; CPAs to sponsor student manuscript contest • Student Use of Helfferich Clarified • New Medical Ethics Course Offered at Ursinus • Field Hockey Winning Ways Return • Booters Offense Sharp • Bear Loss in Final Quarterhttps://digitalcommons.ursinus.edu/grizzlynews/1064/thumbnail.jp
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Low temperature demonstration geothermal power plant in the Raft River Valley
Spitzer IRAC Low Surface Brightness Observations of the Virgo Cluster
We present 3.6 and 4.5 micron Spitzer IRAC imaging over 0.77 square degrees
at the Virgo cluster core for the purpose of understanding the formation
mechanisms of the low surface brightness intracluster light features.
Instrumental and astrophysical backgrounds that are hundreds of times higher
than the signal were carefully characterized and removed. We examine both
intracluster light plumes as well as the outer halo of the giant elliptical
M87. For two intracluster light plumes, we use optical colors to constrain
their ages to be greater than 3 & 5 Gyr, respectively. Upper limits on the IRAC
fluxes constrain the upper limits to the masses, and optical detections
constrain the lower limits to the masses. In this first measurement of mass of
intracluster light plumes we find masses in the range of 5.5 x 10^8 - 4.5 x
10^9 and 2.1 x 10^8 - 1.5 x 10^9 solar masses for the two plumes for which we
have coverage. Given their expected short lifetimes, and a constant production
rate for these types of streams, integrated over Virgo's lifetime, they can
account for the total ICL content of the cluster implying that we do not need
to invoke ICL formation mechanisms other than gravitational mechanisms leading
to bright plumes. We also examined the outer halo of the giant elliptical M87.
The color profile from the inner to outer halo of M87 (160 Kpc) is consistent
with either a flat or optically blue gradient, where a blue gradient could be
due to younger or lower metallicity stars at larger radii. The similarity of
the age predicted by both the infrared and optical colors (> few Gyr) indicates
that the optical measurements are not strongly affected by dust extinction.Comment: 16 pages including appendix, 9 figures, ApJ accepte
Cataclysmic Variables in the First Year of the Zwicky Transient Facility
Using selection criteria based on amplitude, time, and color, we have identified 329 objects as known or candidate cataclysmic variables (CVs) during the first year of testing and operation of the Zwicky Transient Facility. Of these, 90 are previously confirmed CVs, 218 are strong candidates based on the shape and color of their light curves obtained during 3–562 days of observation, and the remaining 21 are possible CVs but with too few data points to be listed as good candidates. Almost half of the strong candidates are within 10 deg of the galactic plane, in contrast to most other large surveys that have avoided crowded fields. The available Gaia parallaxes are consistent with sampling the low mass transfer CVs, as predicted by population models. Our follow-up spectra have confirmed Balmer/helium emission lines in 27 objects, with four showing high-excitation He ii emission, including candidates for an AM CVn, a polar, and an intermediate polar. Our results demonstrate that a complete survey of the Galactic plane is needed to accomplish an accurate determination of the number of CVs existing in the Milky Way
Corotational Instability, Magnetic Resonances and Global Inertial-Acoustic Oscillations in Magnetized Black-Hole Accretion Discs
Low-order, non-axisymmetric p-modes (also referred as inertial-acoustic
modes) trapped in the inner-most region of hydrodynamic accretion discs around
black holes, are plausible candidates for high-frequency quasi-periodic
oscillations (QPOs) observed in a number of accreting black-hole systems. These
modes are subject to global instabilities due to wave absorption at the
corotation resonance (where the wave pattern frequency equals the
disc rotation rate ), when the fluid vortensity,
(where and are the radial
epicyclic frequency and disc surface density, respectively), has a positive
gradient. We investigate the effects of disc magnetic fields on the wave
absorption at corotation and the related wave super-reflection of the
corotation barrier, and on the overstability of disc p-modes. For discs with a
pure toroidal field, the corotation resonance is split into two magnetic
resonances, where the wave frequency in the corotating frame of the fluid,
\tomega=\omega-m\Omega, matches the slow magnetosonic wave frequency.
Significant wave energy/angular momentum absorption occurs at both magnetic
resonances, but with opposite signs. The combined effect of the two magnetic
resonances is to reduce the super-reflection and the growth rate of the
overstable p-modes. We show that even a subthermal toroidal field may suppress
the overstability of hydrodynamic (B=0) p-modes. For accretion discs with mixed
(toroidal and vertical) magnetic fields, two additional Alfven resonances
appear, where \tomega matches the local Alfven wave frequency. They further
reduce the growth rate of p-modes. Our results suggest that in order for the
non-axisymmetric p-modes to be a viable candidate for the observed
high-frequency QPOs, the disc magnetic field must be appreciably subthermal, or
other mode excitation mechanisms are at work.Comment: 21 pages, 11 figures, MNRAS accepte
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