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200 papers

A stochastic model of the chemical enrichment of metal-poor systems by core-collapse (Type II) supernovae is presented, allowing for large-scale mixing of the enriched material by turbulent motions and cloud collisions in the interstellar…

Astrophysics · Physics 2009-11-11 T. Karlsson

Swope Supernova Survey 2017a (SSS17a) was discovered as the first optical counterpart to the gravitational wave event GW170817. Although its light curve on the timescale of weeks roughly matches the expected luminosity and red color of an…

High Energy Astrophysical Phenomena · Physics 2018-03-28 Anthony L. Piro , Juna A. Kollmeier

A number of trends among the properties of exoplanets have become evident in the years since the first one was announced in 1995. One particularly interesting trend began to emerge in 1997 -- the incidence of giant planets correlates with…

Astrophysics · Physics 2008-11-26 Guillermo Gonzalez

Bipolar explosion models for hypernovae (very energetic supernovae), associated with the black hole formation, are presented. The model features are as follows: (1) Fe-peak elements are ejected at high velocities to reach the surface…

Astrophysics · Physics 2009-11-07 K. Maeda , K. Nomoto

The information on Galactic assembly time is imprinted on the chemodynamics of globular clusters. This makes them important probes that help us to understand the formation and evolution of the Milky Way. Discerning between in-situ and…

We present optical and X-ray data for the first object showing strong evidence for being a black hole in a globular cluster. We show the initial X-ray light curve and X-ray spectrum which led to the discovery that this is an extremely…

To constrain the properties of the first stars with the chemical abundance patterns observed in metal-poor stars, one must identify any non-trivial effects that the hydrodynamics of metal dispersal can imprint on the abundances. We use…

Astrophysics of Galaxies · Physics 2015-10-20 Jeremy S. Ritter , Alan Sluder , Chalence Safranek-Shrader , Milos Milosavljevic , Volker Bromm

We argue that primordial black-hole formation must be described by means of extreme-value theory. This is a consequence of the large values of the energy density required to initiate the collapse of black holes in the early Universe and the…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-28 Florian Kuhnel , Dominik J. Schwarz

Most of the ordinary matter in the local Universe has not been converted into stars but resides in a largely unexplored diffuse, hot, X-ray emitting plasma. It pervades the gravitational potentials of massive galaxies, groups and clusters…

Astrophysics of Galaxies · Physics 2020-07-22 Norbert Werner , François Mernier

We show that a subdominant component of dissipative dark matter resembling the Standard Model can form many intermediate-mass black hole seeds during the first structure formation epoch. We also observe that, in the presence of this matter…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-25 Guido D'Amico , Paolo Panci , Alessandro Lupi , Stefano Bovino , Joseph Silk

The investigation of the metal-poor tail in the Galactic bulge provides unique information on the early Milky Way assembly and evolution. A chemo-dynamical analysis of 17 very metal-poor stars (VMP, [Fe/H] $<-2.0$) selected from the…

Except serving as an excellent gift on proper occasions, gold finds applications in life sciences, particularly in diagnostics and therapeutics. These applications were made possible by gold nanoparticles, which differ drastically from…

Materials Science · Physics 2015-06-23 Vitaly Chaban

Since Hawking's 1974 discovery, we expect that a black hole formed by collapse will emit radiation and eventually disappear. Closely related to the information loss puzzle is the challenge to define an objective notion of physical entropy…

High Energy Physics - Theory · Physics 2023-03-31 Bernard S. Kay

The possible topology of quantum fluctuations which take place at the earliest stage of high-energy processes is studied. A new exact solution of Yang-Mills equations with fractional topological charge and carrying a single color is found.

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Makhlin

A thermonuclear explosion triggered by a helium-shell detonation on a carbon-oxygen white dwarf core has been predicted to have strong UV line blanketing at early times due to the iron-group elements produced during helium-shell burning. We…

Pluto's icy surface has changed colour and its atmosphere has swelled since its last closest approach to the Sun in 1989. The thin atmosphere is produced by evaporating ices, and so can also change rapidly, and in particular carbon monoxide…

Earth and Planetary Astrophysics · Physics 2015-05-27 J. S. Greaves , Ch. Helling , P. Friberg

To anyone who has read a scientific journal or even a newspaper in the last six months, it might appear that cosmic gamma-ray bursts hold no more mysteries: they are cosmological, and possibly the most powerful explosions in the Universe.…

Astrophysics · Physics 2007-05-23 K. Hurley

Primordial black holes may owe their origin to the small-scale enhancement of the comoving curvature perturbation generated during inflation. Their mass fraction at formation is markedly sensitive to possible non-Gaussianities in such…

Cosmology and Nongalactic Astrophysics · Physics 2018-03-13 G. Franciolini , A. Kehagias , S. Matarrese , A. Riotto

Metals from Population III (Pop III) supernovae led to the formation of less massive Pop II stars in the early universe, altering the course of evolution of primeval galaxies and cosmological reionization. There are a variety of scenarios…

Astrophysics of Galaxies · Physics 2017-08-02 Ke-Jung Chen , Daniel J. Whalen , Katharina M. J. Wollenberg , Simon C. O. Glover , Ralf S. Klessen

CK Vulpeculae was observed in outburst in 1670-16721, but no counterpart was seen until 1982, when a bipolar nebula was found at its location. Historically, CK Vul has been considered to be a nova (Nova Vul 1670), but a similarity to 'red…

Solar and Stellar Astrophysics · Physics 2015-03-24 Tomasz Kaminski , Karl M. Menten , Romuald Tylenda , Marcin Hajduk , Nimesh A. Patel , Alexander Kraus