1,187 research outputs found
Supernova 1996L: evidence of a strong wind episode before the explosion
Observations of the type II SN 1996L reveal the presence of a slowly
expanding (V~700$ km/s) shell at ~ 10^(16) cm from the exploding star. Narrow
emission features are visible in the early spectra superposed on the normal SN
spectrum. Within about two months these features develop narrow symmetric
P-Cygni profiles. About 100 days after the explosion the light curve suddenly
flattens, the spectral lines broaden and the Halpha flux becomes larger than
what is expected from a purely radioactive model. These events are interpreted
as signatures of the onset of the interaction between the fast moving ejecta
and a slowly moving outer shell of matter ejected before the SN explosion. At
about 300 days the narrow lines disappear and the flux drops until the SN fades
away, suggesting that the interaction phase is over and that the shell has been
swept away. Simple calculations show that the superwind episode started 9 yr
before the SN explosion and lasted 6 yr, with an average dM/dt=10^(-3)
M_solar/yr. Even at very late epochs (up to day 335) the typical forbidden
lines of [OI], CaII], [FeII] remain undetected or very weak. Spectra after day
270 show relatively strong emission lines of HeI. These lines are narrower than
other emission lines coming from the SN ejecta, but broader than those from the
CSM. These high excitation lines are probably the result of non-thermal
excitation and ionization caused by the deposition of the gamma-rays emitted in
the decay of radioactive material mixed in the He layer.Comment: 8 pages, 6 figures, Latex, To appear in M.N.R.A.
Lack of observational evidence for quantum structure of space-time at Plank scales
It has been noted (Lieu & Hillmann, 2002) that the cumulative affect of
Planck-scale phenomenology, or the structure of space-time at extremely small
scales, can be lead to the loss of phase of radiation emitted at large
distances from the observer. We elaborate on such an approach and demonstrate
that such an effect would lead to an apparent blurring of distant
point-sources. Evidence of the diffraction pattern from the HST observations of
SN 1994D and the unresolved appearance of a Hubble Deep Field galaxy at z=5.34
lead us to put stringent limits on the effects of Planck-scale phenomenology.Comment: 12 pages, 3 figures, accepter for ApJ
The Asiago Supernova Catalogue- 10 years after
Ten years after the publication of the previous release, we present a new
edition of the Asiago Supernova Catalogue updated to December 31, 1998 and
containing data for 1447 supernovae and their parent galaxies\footnote{Tables 1
and 2 are only available in electronic form at the CDS via anonymous ftp to
cdsarc.u-strasbg.fr (130.79.128.5) or via
http://cdsweb.u-strasbg.fr/Abstract.html}. In addition to list the data for a
large number of new SNe, we made an effort to search the literature for new
information on past SNe as well. We also tried to update and homogenize the
data for the parent galaxies. To allow a global view of the Catalogue, a few
descriptive figures and a summary table is reported. The present Catalogue is
intended as a large and modern database for statistical studies on the
supernova phenomenon.Comment: 6 pages. To be published in A&A supplement. Enclosed as postscript
files are the full lists in chronological (snean.ps) and R.A. (snear.ps)
order (to be published only in electronic form.
Independent circuits in basal ganglia and cortex for the processing of reward and precision feedback
In order to understand human decision making it is necessary to understand
how the brain uses feedback to guide goal-directed behavior. The ventral
striatum (VS) appears to be a key structure in this function, responding
strongly to explicit reward feedback. However, recent results have also shown
striatal activity following correct task performance even in the absence of
feedback. This raises the possibility that, in addition to processing external
feedback, the dopamine-centered reward circuit might regulate endogenous
reinforcement signals, like those triggered by satisfaction in accurate task
performance. Here we use functional magnetic resonance imaging (fMRI) to test
this idea. Participants completed a simple task that garnered both reward
feedback and feedback about the precision of performance. Importantly, the
design was such that we could manipulate information about the precision of
performance within different levels of reward magnitude. Using parametric
modulation and functional connectivity analysis we identified brain regions
sensitive to each of these signals. Our results show a double dissociation:
frontal and posterior cingulate regions responded to explicit reward but were
insensitive to task precision, whereas the dorsal striatum - and putamen in
particular - was insensitive to reward but responded strongly to precision
feedback in reward-present trials. Both types of feedback activated the VS, and
sensitivity in this structure to precision feedback was predicted by
personality traits related to approach behavior and reward responsiveness. Our
findings shed new light on the role of specific brain regions in integrating
different sources of feedback to guide goal-directed behavior
Supernova Classes and Subclasses
The discovery of many objects with unprecedented, amazing observational
characteristics caused the last decade to be the most prolific period for the
supernova research. Many of these new supernovae are transitional objects
between existing classes, others well enter within the defined classes, but
still show unique properties. This makes the traditional classification scheme
inadequate to take into account the overall SN variety and, consequently,
requires the introduction of new subclasses.Comment: 10 pages, 2 figure, review for "Supernova 1987A: 20 Years After:
Supernovae and Gamma-Ray Bursters" AIP, New York, eds. S. Immler, K.W.
Weiler, and R. McCra
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