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Related papers: Rayed craters on Dione: Implication for the domina…

200 papers

If dark matter annihilates to light quarks in the core of the Sun, then a flux of 236 MeV neutrinos will be produced from the decay of stopped kaons. We consider strategies for DUNE to not only observe such a signal, but to determine the…

High Energy Physics - Phenomenology · Physics 2017-10-12 Carsten Rott , Seongjin In , Jason Kumar , David Yaylali

The ring system and small satellites of Neptune were discovered during Voyager 2 flyby in 1989 (Smith et al.1989). In this work we analyse the diffusion maps which can give an overview of the system. As a result we found the width of…

Earth and Planetary Astrophysics · Physics 2020-03-06 D. M. Gaslac Gallardo , S. M. Giuliatti Winter , G. Madeira , M. A. Muñoz-Gutiérrez

Planet formation takes place in protoplanetary discs around young T-Tauri stars. PDS 70 is one of the first confirmed examples of a system where the planets are currently forming in gaps in the disc, and can be directly imaged. One of the…

Solar and Stellar Astrophysics · Physics 2024-05-24 Simon R. G. Joyce , John P. Pye , Jonathan D. Nichols , Richard Alexander , Manuel Gudel , David Barrado

Accretion of interstellar material by a magnetized, slowly rotating isolated neutron star is discussed. We show that the average persistent X-ray luminosity of these objects is unlikely to exceed 4x10^26 erg/s. They can also appear as X-ray…

Astrophysics · Physics 2007-05-23 N. R. Ikhsanov , P. L. Biermann

The hypothesis of a recent origin of Saturn's rings and its mid-sized moons is actively debated. It was suggested that a proto-Rhea and a proto-Dione might have collided recently, giving birth to the modern system of mid-sized moons. It is…

Earth and Planetary Astrophysics · Physics 2017-07-04 Ryuki Hyodo , Sébastien Charnoz

We investigate under what circumstances an embedded planet in a protoplanetary disc may sculpt the dust distribution such that it observationally presents as a `transition' disc. We concern ourselves with `transition' discs that have large…

Earth and Planetary Astrophysics · Physics 2015-06-19 James E. Owen

We have worked for some time on a model for dark matter, in which dark matter consists of small bubbles of a new speculated type of vacuum, which are pumped up by some ordinary matter such as diamond, so as to resist the pressure of the…

High Energy Physics - Phenomenology · Physics 2023-11-28 H. B. Nielsen , Colin D. Froggatt

The 2009 Lunar CRater Observation and Sensing Satellite (LCROSS) impact mission detected water ice absorption using spectroscopic observations of the impact-generated debris plume taken by the Shepherding Spacecraft, confirming an existing…

Earth and Planetary Astrophysics · Physics 2020-09-14 Kristen M. Luchsinger , Nancy J. Chanover , Paul D. Strycker

(Abridged) A numerical model of a circumstellar debris disk is developed and applied to observations of the circumstellar dust orbiting beta Pictoris. The model accounts for the rates at which dust is produced by collisions among unseen…

Earth and Planetary Astrophysics · Physics 2015-05-19 Joseph M. Hahn

Galactic cosmic rays are a ubiquitous source of ionisation of the interstellar gas, competing with UV and X-ray photons as well as natural radioactivity in determining the fractional abundance of electrons, ions and charged dust grains in…

High Energy Astrophysical Phenomena · Physics 2018-06-27 Marco Padovani , Alexei V. Ivlev , Daniele Galli , Paola Caselli

Measuring the cosmic ray flux over timescales comparable to the age of the solar system, $\sim 4.5\,$Gyr, could provide a new window on the history of the Earth, the solar system, and even our galaxy. We present a technique to indirectly…

High Energy Physics - Phenomenology · Physics 2020-12-01 Johnathon R. Jordan , Sebastian Baum , Patrick Stengel , Alfredo Ferrari , Maria Cristina Morone , Paola Sala , Joshua Spitz

Cosmic rays are an essential ingredient in the evolution of the interstellar medium, as they dominate the ionisation of the dense molecular gas, where stars and planets form. However, since they are efficiently scattered by the galactic…

Astrophysics of Galaxies · Physics 2014-09-05 Solenn Vaupré , Pierre Hily-Blant , Cecilia Ceccarelli , Guillaume Dubus , Stefano Gabici , Thierry Montmerle

The $\mu$ and $\nu$ rings of Uranus form a secondary ring-moon system with the satellites Puck, Mab,Portia, and Rosalind. These rings are tenuous and dominated by micrometric particles, which can be strongly disturbed by the solar radiation…

Earth and Planetary Astrophysics · Physics 2013-07-12 R. Sfair

We have carried out a sensitive search for gas emission lines at infrared and millimeter wavelengths for a sample of 15 young sun-like stars selected from our dust disk survey with the Spitzer Space Telescope. We have used mid-infrared…

White dwarfs are the end state of most stars, including the Sun, after they exhaust their nuclear fuel. Between 1/4 and 1/2 of white dwarfs have elements heavier than helium in their atmospheres, even though these elements should rapidly…

A star enshrouded in a Dyson sphere with high covering fraction may manifest itself as an optically subluminous object with a spectrophotometric distance estimate significantly in excess of its parallax distance. Using this criterion, the…

Solar and Stellar Astrophysics · Physics 2018-08-01 Erik Zackrisson , Andreas J. Korn , Ansgar Wehrhahn , Johannes Reiter

High energy radiation from a planet host star can have strong influence on the final habitability of a system through several mechanisms. In this context we have constructed a catalogue containing the X-ray luminosities, as well as basic…

Earth and Planetary Astrophysics · Physics 2019-01-09 Kristina Monsch , Barbara Ercolano , Giovanni Picogna , Thomas Preibisch , Markus Michael Rau

Neutron stars, with their strong surface gravity, have interestingly short timescales for the sedimentation of heavy elements. Recent observations of unstable thermonuclear burning (observed as X-ray bursts) on the surfaces of slowly…

Astrophysics · Physics 2008-11-26 Fang Peng , Edward F. Brown , James W. Truran

We report cosmic ray ionization rates towards ten reddened stars studied within the framework of the EDIBLES (ESO Diffuse Interstellar Bands Large Exploration Survey) program, using the VLT-UVES. For each sightline, between 2 and 10…