274 research outputs found
Extreme Plasma Astrophysics
This is a science white paper submitted to the Astro-2020 and Plasma-2020
Decadal Surveys. The paper describes the present status and emerging
opportunities in Extreme Plasma Astrophysics -- a study of
astrophysically-relevant plasma processes taking place under extreme conditions
that necessitate taking into account relativistic, radiation, and QED effects.Comment: A science white paper submitted to the Astro-2020 and Plasma-2020
Decadal Surveys. 7 pages including cover page and references. Paper updated
in late March 2019 to include a several additional co-authors and references,
and a few small change
110 Minima timings of ultra-short orbital period eclipsing binaries
We present 110 times of minima of 7 ultra-short orbital period eclipsing binaries
The hunt for extraterrestrial high-energy neutrino counterparts
The origin of Petaelectronvolt (PeV) astrophysical neutrinos is fundamental
to our understanding of the high-energy Universe. Apart from the technical
challenges of operating detectors deep below ice, oceans, and lakes, the
phenomenological challenges are even greater than those of gravitational waves;
the sources are unknown, hard to predict, and we lack clear signatures.
Neutrino astronomy therefore represents the greatest challenge faced by the
astronomy and physics communities thus far. The possible neutrino sources range
from accretion disks and tidal disruption events, to relativistic jets and
galaxy clusters with blazar TXS~0506+056 the most compelling association thus
far. Since that association, immense effort has been put into proving or
disproving that jets are indeed neutrino emitters, but to no avail. By
generating simulated neutrino counterpart samples, we explore the potential of
detecting a significant correlation of neutrinos with jets from active galactic
nuclei. We find that, given the existing challenges, even our best experiments
could not have produced a result. Larger programs over the next few
years will be able to detect a significant correlation only if the brightest
radio sources, rather than all jetted active galactic nuclei, are neutrino
emitters. We discuss the necessary strategies required to steer future efforts
into successful experiments.Comment: 8 pages, 1 figure, 1 table, accepted for publication in A&
Fatty acid-related modulations of membrane fluidity in cells: detection and implications
Metabolic homeostasis of fatty acids is complex and well-regulated in all organisms. The biosynthesis of saturated fatty acids (SFA) in mammals provides substrates for ?-oxidation and ATP production. Monounsaturated fatty acids (MUFA) are products of desaturases that introduce a methylene group in cis geometry in SFA. Polyunsaturated fatty acids (n-6 and n-3 PUFA) are products of elongation and desaturation of the essential linoleic acid and ?-linolenic acid, respectively. The liver processes dietary fatty acids and exports them in lipoproteins for distribution and storage in peripheral tissues. The three types of fatty acids are integrated in membrane phospholipids and determine their biophysical properties and functions. This study was aimed at investigating effects of fatty acids on membrane biophysical properties under varying nutritional and pathological conditions, by integrating lipidomic analysis of membrane phospholipids with functional two-photon microscopy (fTPM) of cellular membranes. This approach was applied to two case studies: first, pancreatic beta-cells, to investigate hormetic and detrimental effects of lipids. Second, red blood cells extracted from a genetic mouse model defective in lipoproteins, to understand the role of lipids in hepatic diseases and metabolic syndrome and their effect on circulating cells
Aperture effects on the oxygen abundance determinations from CALIFA data
This paper aims at providing aperture corrections for emission lines in a
sample of spiral galaxies from the Calar Alto Legacy Integral Field Area Survey
(CALIFA) database. In particular, we explore the behavior of the
log([OIII]5007/Hbeta)/([NII]6583/Halpha) (O3N2) and log[NII]6583/Halpha (N2)
flux ratios since they are closely connected to different empirical
calibrations of the oxygen abundances in star forming galaxies.
We compute median growth curves of Halpha, Halpha/Hbeta, O3N2 and N2 up to
2.5R_50 and 1.5 disk R_eff. The growth curves simulate the effect of observing
galaxies through apertures of varying radii. The median growth curve of the
Halpha/Hbeta ratio monotonically decreases from the center towards larger
radii, showing for small apertures a maximum value of ~10% larger than the
integrated one. The median growth curve of N2 shows a similar behavior,
decreasing from the center towards larger radii. No strong dependence is seen
with the inclination, morphological type and stellar mass for these growth
curves. Finally, the median growth curve of O3N2 increases monotonically with
radius. However, at small radii it shows systematically higher values for
galaxies of earlier morphological types and for high stellar mass galaxies.
Applying our aperture corrections to a sample of galaxies from the SDSS
survey at 0.02<=z<=0.3 shows that the average difference between fiber-based
and aperture corrected oxygen abundances, for different galaxy stellar mass and
redshift ranges, reaches typically to ~11%, depending on the abundance
calibration used. This average difference is found to be systematically biased,
though still within the typical uncertainties of oxygen abundances derived from
empirical calibrations. Caution must be exercised when using observations of
galaxies for small radii (e.g. below 0.5R_eff) given the high dispersion shown
around the median growth curves.Comment: Accepted for publication in Ap
Surface density of the young cluster IC 348 in the Perseus molecular cloud
The IC 348 young star cluster contains more than 300 confirmed members. It is
embedded in the Perseus molecular cloud, making any clustering analysis subject
to an extinction bias. In this work, we derive the extinction map of the cloud
and revisit the content of IC 348 through a statistical approach that uses the
2MASS data. Our goal was to address the question of the completeness of IC 348
and of young clusters in general. We performed a combined analysis of the star
color and density in this region, in order to establish the surface density map
of the cluster. We reached the conclusion that IC 348 has structures up to 25'
from the cluster center, and we estimate that about 40 members brighter than
Ks=13 mag are still unidentified. Although we cannot use our statistical method
to identify these new members individually, the surface density map gives a
strong indication of their actual location. They are distributed in the outer
regions of the cluster, where very few dedicated observations have been made so
far, which is probably why they escaped previous identification. In addition,
we propose the existence of a new embedded cluster associated to the infrared
source MSX6C G160.2784-18.4216, about 38' south of IC 348.Comment: 5 pages, 5 figures, accepted for publication in A&
Whole exome sequence analysis reveals a homozygous mutation in PNPLA2 as the cause of severe dilated cardiomyopathy secondary to neutral lipid storage disease.
Accepted manuscript 12 month embargo, pre-print immediately
- …