Results 131 to 140 of about 260 (145)

Gravitational-wave astronomy: delivering on the promises. [PDF]

Philos Trans A Math Phys Eng Sci, 2018
Schutz BF.
europepmc   +1 more source

All-Glass 100 mm Diameter Visible Metalens for Imaging the Cosmos. [PDF]

ACS Nano
Park JS, Lim SWD, Amirzhan A, Kang H, Karrfalt K, Kim D, Leger J, Urbas A, Ossiander M, Li Z, Capasso F.   +10 more
europepmc   +1 more source

Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster. [PDF]

Nat Astron
Pearlman AB, Scholz P, Bethapudi S, Hessels JWT, Kaspi VM, Kirsten F, Nimmo K, Spitler LG, Fonseca E, Meyers BW, Stairs IH, Tan CM, Bhardwaj M, Chatterjee S, Cook AM, Curtin AP, Dong FA, Eftekhari T, Gaensler BM, Güver T, Kaczmarek J, Leung C, Masui KW, Michilli D, Prince TA, Sand KR, Shin K, Smith KM, Tendulkar SP.   +28 more
europepmc   +1 more source

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Sub-percent binary star masses and distances from interferometric observations

Proceedings of the International Astronomical Union, 2022
AbstractOur knowledge of stellar evolution relies on constraints provided by measurements of the physical stellar properties such as the mass, effective temperature, and radii. The most fundamental parameter, the stellar mass, is rarely available or has a low accuracy, providing poor constraints on the stellar structure and evolution.
openaire   +1 more source

Interferometric studies of disk-eclipsed binary star systems

SPIE Proceedings, 2016
As sky surveys continue to document an increasing number of transient celestial phenomena, an intriguing subset of objects are emerging that show variations in brightness, interpreted as the transit of a circumstellar disk in front of a companion star in a binary system.
openaire   +1 more source

FINEST - Finder and observer of neutron star binary coalescence

1997
A new concept for a space-based, interferometric gravitational wave detector is envisaged called FINEST targeted at observing medium-frequency gravitational waves (10-1 to 103 Hz). Established technologies that have been developed for ground-based detectors along with those being developed for space-based detectors are utilised.
Roberts, Peter; id_orcid 0000-0001-9160-777X, Dolesi, Rita, Maraner, Antonella, Kaltenegger, Lisa, Lechner, Christiane, Nieke, Jens, Wilhelm, Rainer, Peterseim, Michael   +7 more
openaire   +2 more sources

Interferometric radii of bright Kepler stars with the CHARA Array: θ Cygni and 16 Cygni A and B

Monthly Notices of the Royal Astronomical Society, 2013
John D Monnier, Timothy White, László Stürmann   +2 more
exaly  

Speckle interferometric measurements of binary stars. IV

Astrophysical Journal, 1979
H A Mcalister
exaly  

Interferometric diameters of five evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array

Monthly Notices of the Royal Astronomical Society, 2018
Daniel Huber, Anders Bo Justesen, VÍCTOR Aguirre Børsen-Koch   +2 more
exaly  

Spectro-interferometric observations of a sample of Be stars

Astronomy and Astrophysics, 2019
Michel Cure, Catalina Arcos, Lydia Cidale   +2 more
exaly