Constraining the neutron star equation of state using Pulse Profile Modeling [PDF]
, 2019 One very promising technique for measuring the dense matter Equation of State exploits hotspots that form on the neutron star surface due to the pulsar mechanism, accretion streams, or during thermonuclear explosions in the neutron star ocean.
Watts, Anna L.
core +3 more sources
Space Instrumentation: Imaging Interferometry [PDF]
, 1999 A short overview on aperture synthesis in space for the non ...
arxiv +1 more source
Implementation of the trigger algorithm for the NEMO project [PDF]
, 2007 We describe the implementation of trigger algorithm specifically tailored on the characteristics of the neutrino telescope NEMO. Extensive testing against realistic simulations shows that, by making use of the uncorrelated nature of the noise produced ...
Brescia, M., d'Angelo, G., Riccio, G.
core +1 more source
Stellar laboratories: new Ge V and Ge VI oscillator strengths and their validation in the hot white dwarf RE 0503–289 [PDF]
, 2012 Context. State-of-the-art spectral analysis of hot stars by means of non-LTE model-atmosphere techniques has arrived at a high level of sophistication. The analysis of high-resolution and high-S/N spectra, however, is strongly restricted by the lack of ...
T. Rauch +22 more
semanticscholar +1 more source
Statistical analysis of the trigger algorithm for the NEMO project [PDF]
, 2007 We discuss the performances of a trigger implemented for the planned neutrino telescope NEMO. This trigger seems capable to discriminate between the signal and the strong background introduced by atmospheric muons and by the beta decay of the K-40 nuclei
Brescia, M., D'Angelo, G., Riccio, G.
core +1 more source
Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics [PDF]
, 2001 Cosmic microwave background (CMB) determinations of the baryon-to-photon ratio $\eta \propto \Omega_{\rm baryon} h^2$ will remove the last free parameter from (standard) big bang nucleosynthesis (BBN) calculations. This will make BBN a much sharper probe
Balbi +48 more
core +3 more sources
Internal kinematics of modelled interacting disc galaxies [PDF]
, 2006 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany-/-Abstract. We present an investigation of galaxy-galaxy interactions and their effects on the velocity fields of discgalaxies in combined N-body/hydrodynamic simulations,
T. Kronberger +13 more
semanticscholar +1 more source
Frontiers of Astrophysics - Workshop Summary
, 1997 We summarize recent results presented in the astrophysics session during a conference on ``Frontiers of Contemporary Physics''. We will discuss three main fields (High-Energy Astrophysics, Relativistic Astrophysics, and Cosmology), where Astrophysicists ...
Biermann, Peter L., Falcke, Heino
core +2 more sources
A Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology [PDF]
, 2006 A relativistic modified gravity (MOG) theory leads to a self-consistent, stable gravity theory that can describe the solar system, galaxy and clusters of galaxies data and cosmology.Comment: 16 pages. Latex file. Talk given at the International Workshop "
Anderson J. D. +5 more
core +2 more sources
Direct determination of oxygen abundances in line-emitting star-forming galaxies at intermediate redshift [PDF]
, 2015 We present a sample of 22 blue ($(B-V)_{AB}
J. M. P'erez +16 more
semanticscholar +1 more source