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相关论文: Interferometry in astrophysics as a roadmap for in…

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Astrometry is a powerful technique in astrophysics to measure three-dimensional positions of stars and other astrophysical objects, including exoplanets and the gravitational influence they have on each other. Interferometric astrometry is…

天体物理仪器与方法 · 物理学 2018-12-10 Michael J. Ireland , Julien Woillez

After decades of efforts, optical long-baseline interferometry has become a mainstream observational technique in terms of operation robustness and user friendliness. Interferometry has opened a new observational window, enabling…

太阳与恒星天体物理 · 物理学 2025-12-02 H. Sana E. Bordier , K. Deshmukh , A. J. Frost , A. Keskar , C. Lanthermann , R. R. Lefever , L. Mahy , A. A. C. Sander , T. Shenar , F. Tramper

The space-time correlations of streams of photons can provide fundamentally new channels of information about the Universe. Today's astronomical observations essentially measure certain amplitude coherence functions produced by a source.…

天体物理仪器与方法 · 物理学 2009-03-03 C. Barbieri , M. K. Daniel , W. J. de Wit , D. Dravins , H. Jensen , P. Kervella , S. Le Bohec , F. Malbet , P. Nunez , J. P. Ralston , E. N. Ribak

Long-baseline interferometry at optical and near-infrared wavelengths is an emerging technology which is quickly becoming a useful tool to investigate stellar atmospheres and to compare observations with models. Stellar atmosphere models…

天体物理学 · 物理学 2007-05-23 Markus Wittkowski

MHD Turbulence is a critical component of the current paradigms of star formation, particle transport, magnetic reconnection and evolution of the ISM. Progress on this difficult subject is made via numerical simulations and observational…

星系天体物理 · 物理学 2011-05-06 Blakesley Burkhart , Alex Lazarian

An introduction to the theory and practical aspects of infrared interferometry is given in the context of the study of massive young stellar objects. Basic interferometric concepts, as well as observable quantities and their use, are…

太阳与恒星天体物理 · 物理学 2014-02-17 Paul A. Boley

While it is well known that most massive stars are found to be part of binary or multiple systems, an accurate characterization of the statistical properties of these multiple objects is still lacking. In the present talk, we will review…

太阳与恒星天体物理 · 物理学 2009-06-30 H. Sana , J. -B. Le Bouquin

Interferometry has brought many new constraints in optical astronomy in the recent years. A major leap in this field is the opening of large interferometric facilities like the Very Large Telescope Interferometer and the Keck Interferometer…

天体物理学 · 物理学 2007-05-23 F. Malbet

Optical long-baseline interferometry is a unique and powerful technique for astronomical research. Since 2004, optical interferometers have produced an increasing number of scientific papers covering various fields of astrophysics. As…

天体物理仪器与方法 · 物理学 2018-05-28 D. Defrère , C. Aerts , M. Kishimoto , P. Léna

Optical interferometry provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Through direct observation of rotationally distorted photospheres at sub-milliarcsecond scales, we are now able to…

太阳与恒星天体物理 · 物理学 2012-04-13 Gerard T. van Belle

Increasingly sophisticated observational tools and techniques are now being developed for probing the nature of interstellar turbulence. At the same time, theoretical advances in understanding the nature of turbulence and its effects on the…

天体物理学 · 物理学 2009-11-10 Mark Heyer , Ellen Zweibel

Future large arrays of telescopes, used as intensity interferometers, can be used to image the surfaces of stars with unprecedented angular resolution. Fast-rotating, hot stars are particularly attractive targets for intensity…

天体物理仪器与方法 · 物理学 2015-09-09 Paul D. Nunez , Armando Domiciano de Souza

The present status of the use of two-particle intensity interferometry as a diagnostic tool to study the space-time dynamics of intermediate energy heavy ion collisions is examined. Calculations for the two-proton and two-pion correlation…

核理论 · 物理学 2009-10-22 Wolfgang Bauer

MHD Turbulence is a critical component of the current paradigms of star formation, particle transport, magnetic reconnection and evolution of the ISM, to name just a few. Progress on this difficult subject is made via numerical simulations…

星系天体物理 · 物理学 2015-05-27 Blakesley Burkhart , Alex Lazarian

We report on a considerable improvement in the technique of measuring multiparticle correlations via integrals over correlation functions. A modification of measures used in the characterization of chaotic dynamical sytems permits fast and…

高能物理 - 唯象学 · 物理学 2009-10-22 H. C. Eggers , P. Lipa , P. Carruthers , B. Buschbeck

We propose an innovative scheme exploiting discrete diffraction in a two dimensional array of coupled waveguides to determine the phase and amplitude of the mutual correlation function between any pair of three telescopes of an…

光学 · 物理学 2011-03-28 Stefano Minardi , Thomas Pertsch

Modern optical spectrographs and optical interferometers push the limits in the spectral and spatial regime, providing important new tools for the exploration of the universe. In this contribution I outline the complementary nature of…

太阳与恒星天体物理 · 物理学 2015-06-18 Stefan Kraus

This paper serves as a reference on how to estimate the parameters of binary stars and how to combine multiple techniques, namely astrometry, interferometry and radial velocities.

太阳与恒星天体物理 · 物理学 2015-10-29 Daniel Bonneau , Florentin Millour , Anthony Meilland

The study of molecular physics using ultracold gases has provided a unique probe into the fundamental properties of nature and offers new tools for quantum technologies. In this article we outline how the use of a space environment to study…

I present a discussion of fundamental stellar parameters and their observational determination in the context of interferometric measurements with current and future optical/infrared interferometric facilities. Stellar parameters and the…

天体物理学 · 物理学 2007-05-23 M. Wittkowski
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