64,206 research outputs found
Long-term IR Photometry of Seyferts
Long-term (up to 10000d) monitoring has been undertaken for 41 Seyferts in
the near-IR (JHKL). All but 2 showed variability, with K ampl in the range <0.1
to > 1.1 mags. The timescale for detectable change is from about one week to a
few years. A simple cross-correlation study shows evidence for delays of up to
several hundred days between the variations seen at the shortest wavelengths
and the longest in many galaxies. In particular, the data for F9 now extend to
twice the interval covered earlier and the delay between its UV and IR outputs
persists. An analysis of the fluxes shows that, for any given galaxy, the
colours of the variable component are usually independent of the level of
activity. The state of activity can be parameterized. Taken over the whole
sample, the colours of the variable components fall within moderately narrowly
defined ranges. In particular, the H-K colour is appropriate to a black body of
temperature 1600K. The H-K excess for a heavily reddened nucleus can be
determined and used to find E_{B-V}, which can be compared to the values found
from the visible region broad line fluxes. Using flux-flux diagrams, the flux
within the aperture from the underlying galaxy can often be determined without
the need for model surface brightness profiles. In many galaxies it is apparent
that here must be an additional constant contribution from warm dust.Comment: Better quality available from ftp://ftp.saao.ac.za/pub/isg/seyf.pd
Period-magnitude relations for M giants in Baade's Window NGC6522
A large and complete sample of stars with K < 9.75 in the NGC6522 Baade's
Window is examined using light curves from MACHO and IJK from DENIS. All 4 of
the sequences ABCD in the K vs logP diagram of the LMC are seen in the Bulge.
The Bulge sequences however show some differences from the Magellanic Clouds.
The sequences may be useful as distance indicators. A new diagram of the
frequency of late-type variables is presented. The catalogued SR variables of
the solar nbd are found to be a subset of the total of SRs, biased towards
large amplitude.Comment: 11 pages 11 fig
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Glioma through the looking GLASS: molecular evolution of diffuse gliomas and the Glioma Longitudinal Analysis Consortium.
Adult diffuse gliomas are a diverse group of brain neoplasms that inflict a high emotional toll on patients and their families. The Cancer Genome Atlas and similar projects have provided a comprehensive understanding of the somatic alterations and molecular subtypes of glioma at diagnosis. However, gliomas undergo significant cellular and molecular evolution during disease progression. We review the current knowledge on the genomic and epigenetic abnormalities in primary tumors and after disease recurrence, highlight the gaps in the literature, and elaborate on the need for a new multi-institutional effort to bridge these knowledge gaps and how the Glioma Longitudinal Analysis Consortium (GLASS) aims to systemically catalog the longitudinal changes in gliomas. The GLASS initiative will provide essential insights into the evolution of glioma toward a lethal phenotype, with the potential to reveal targetable vulnerabilities and, ultimately, improved outcomes for a patient population in need
The 2-Ranks of Hyperelliptic Curves with Extra Automorphisms
This paper examines the relationship between the automorphism group of a hyperelliptic curve defined over an algebraically closed field of characteristic two and the 2-rank of the curve. In particular, we exploit the wild ramification to use the Deuring-Shafarevich formula in order to analyze the ramification of hyperelliptic curves that admit extra automorphisms and use this data to impose restrictions on the genera and 2-ranks of such curves. We also show how some of the techniques and results carry over to the case where our base field is of characteristic p \u3e 2
Coble and Eisenhart: Two Gettysburgians Who Led Mathematics
In 1895, there were 134 students at Gettysburg College, which was then called Pennsylvania College. Of these students, two of them went on to become president of the American Mathematical Society. In this article, we look at the lives of these two men, Arthur Coble and Luther Eisenhart, and their contributions to mathematics and higher education, as well as look at what mathematics was like at Gettysburg at the end of the nineteenth century
Composition of Integers with Bounded Parts
In this note, we consider ordered partitions of integers such that each entry is no more than a fixed portion of the sum. We give a method for constructing all such compositions as well as both an explicit formula and a generating function describing the number of k-tuples whose entries are bounded in this way and sum to a fixed value g
Life After Calculus: 20 Years Later
In 1996 Math Horizons interviewed a group of students at the Joint Mathematics Meetings; now, 20 years later, one of those students, Darren Glass, interviews another group of students
Critical Groups of Graphs with Dihedral Actions II
In this paper we consider the critical group of finite connected graphs which admit harmonic actions by the dihedral group Dn, extending earlier work by the author and Criel Merino. In particular, we show that the critical group of such a graph can be decomposed in terms of the critical groups of the quotients of the graph by certain subgroups of the automorphism group. This is analogous to a theorem of Kani and Rosen which decomposes the Jacobians of algebraic curves with a Dn-action
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