Results 21 to 30 of about 351 (182)
Ultra wide‐field infrared astronomy in Antarctica
Astronomische Nachrichten, Volume 344, Issue 8-9, October-November 2023., 2023 The science enabled by the deep and high‐cadence survey that will be performed by the Vera Rubin Observatory has led to an increase of survey and follow‐up capabilities around the world. The infrared, has however, not match this growth due to the challenges caused by the atmospheric and the cost of large detector arrays.
Tony Travouillon +6 more
wiley +1 more source
Characteristic Features of Gravitational Wave Lensing as Probe of Lens Mass Model
Annalen der Physik, Volume 535, Issue 6, June 2023., 2023 The gravitational lensing of gravitational waves is an expanding field in astronomy and cosmology. It might contribute to solving many different issue in these fields. To exploit its potential, first of all, one needs to recognize and model a gravitational wave event properly.
Paolo Cremonese +2 more
wiley +1 more source
The road toward imaging a black hole: A personal perspective
Natural Sciences, Volume 2, Issue 4, October 2022., 2022 The article describes the authors personal journey towards developig the Event Horizon Telescope and the first image of a black hole. Left: predcition made by the author and collaborators proposing the black hole imaging in 2000. Right: the two images observed and published by the Event Horizon Telescope in 2019 and 2022.
Heino Falcke
wiley +1 more source
Identifying interesting planetary systems for future X‐ray observations
Astronomische Nachrichten, Volume 343, Issue 4, May 2022., 2022 Abstract X‐ray observations of star–planet systems are important to grow our understanding of exoplanets; these observations allow for studies of photoevaporation of the exoplanetary atmosphere, and in some cases even estimations of the size of the outer planetary atmosphere.
Grace Foster, Katja Poppenhaeger
wiley +1 more source
MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert
The Astronomical Journal, 2023 We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass.
Greg Olmschenk +82 more
doaj +1 more source
Effervescence‐Inspired Self‐Healing Plastrons for Long‐Term Immersion Stability
Advanced Functional Materials, Volume 32, Issue 4, January 19, 2022., 2022 Underwater performance of superhydrophobic/superamphiphobic surfaces relies on the robustness and durability of the gas‐layer (plastron). A simple and scalable technique of effervescence‐inspired on‐demand plastron repair is presented. Surfaces do not suffer from any performance‐losses even after 2 months of continuous immersion.
William S. Y. Wong, Doris Vollmer
wiley +1 more source
Comparison of Rutherford's atomic model with the Standard Model of particle physics and other models
Journal of the Royal Society of New Zealand, Volume 51, Issue 3-4, Page 538-556, September ‐ December 2021., 2021 ABSTRACT Ernest Rutherford is known almost universally as the discoverer of the structure of the atom. He is less well known for his discovery of the proton. Even less well known is a set of hypotheses on the structure of matter that was proposed by Newton 300 years ago.
Philip Yock
wiley +1 more source
The Fundamental Connections between the Solar System and Exoplanetary Science
Journal of Geophysical Research: Planets, Volume 126, Issue 2, February 2021., 2021 Abstract Over the past several decades, thousands of planets have been discovered outside our Solar System. These planets exhibit enormous diversity, and their large numbers provide a statistical opportunity to place our Solar System within the broader context of planetary structure, atmospheres, architectures, formation, and evolution.
Stephen R. Kane +9 more
wiley +1 more source
A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
Advances in High Energy Physics, Volume 2021, Issue 1, 2021., 2021 The possibility of strange stars mixed with dark energy to be one of the candidates for dark energy stars is the main issue of the present study. Our investigation shows that quark matter atcs as dark energy after a certain yet unknown critical condition inside the quark stars.
Theophanes Grammenos +5 more
wiley +1 more source
Mass Determination with Gravitational Microlensing [PDF]
The Astrophysical Journal, 1996 19 pages in postscript (four figures included), submitted to ...
Mao, Shude, Paczyński, Bohdan
openaire +2 more sources