Results 71 to 80 of about 1,532,155 (277)

A Multiwavelength Light-curve Analysis of the Classical Nova V392 Per: Optical Contribution from an Irradiated Accretion Disk during the Nova Wind Phase

open access: yesThe Astrophysical Journal
The classical nova V392 Per 2018 is characterized by a very fast optical decline, a long binary orbital period of 3.23 days, detection of GeV gamma rays, and almost identical decay trends of the B , V , and I _C light curves.
Izumi Hachisu, Mariko Kato
doaj   +1 more source

A Very-High-Energy Gamma-Ray View of the Transient Sky

open access: yesUniverse
The development of the latest generation of Imaging Atmospheric Cherenkov Telescopes (IACTs) over recent decades has led to the discovery of new extreme astrophysical phenomena in the very-high-energy (VHE, E > 100 GeV) gamma-ray regime.
Alessandro Carosi, Alicia López-Oramas
doaj   +1 more source

Artes Novae

open access: yes, 2018
Fondée en mars 2018, Artes Novae est l'association des jeunes chercheur(e)s en archéologie et histoire de l'art du Moyen Âge et de la Renaissance, actifs en Île-de-France.
Artes Novae
core  

Bidirectional Soft Catalysts for Improved Power Performance of Li‐S Batteries

open access: yesAdvanced Science, EarlyView.
A soft polymer‐metal catalyst is integrated into the binder to create a catalytically active microenvironment that accelerates bidirectional sulfur redox kinetics in lithium‐sulfur batteries. A model polyvinyl alcohol‐Cu catalyst enables high areal capacities at demanding current densities and stable cycling in pouch‐cell prototypes at 0.5 C, achieving
Maleesha M. Nishshanke   +7 more
wiley   +1 more source

Prospects for Observing Astrophysical Transients with Gigaelectronvolt Neutrinos

open access: yesThe Astrophysical Journal
Although Cherenkov detectors of high-energy neutrinos in ice and water are often optimized to detect teraelectronvolt–petaelectronvolt neutrinos, they may also be sensitive to transient neutrino sources in the 1–100 GeV energy range.
Angelina Sherman   +4 more
doaj   +1 more source

The hybrid Nova Vul 2024 (=V615 Vul)

open access: yesAstronomy & Astrophysics
Context. Among galactic novae, many remain poorly characterized due to heterogeneous data, observational challenges, or heavy reddening along the Galactic plane.
Valisa P., Munari U., Albanese I.
doaj   +1 more source

Pięćdziesiąt lat polskich badań archeologicznych w Novae [PDF]

open access: yes, 2012
Recenzja książki: T. Derda, P. Dyczek, J. Kolendo (red.), Novae: Legionary Fortress and Late Antique Town, I: A Companion on the Study of Novae, Wydawnictwo Ośrodka Badań nad Antykiem Europy Południowo-Wschodniej UW, Warsaw 2008 [2009]Recenzja książki: T.
Duch, Michał
core   +2 more sources

Magnetic Water Cleaning of Estrogens via Tight yet Dynamic Binding to Nanoparticles

open access: yesAdvanced Science, EarlyView.
Micropollution is one of the big challenges humanity faces with estrogen hormones being emerging pollutants of concern. Here, a supramolecular design strategy is presented that generates a simple nano‐adsorbent material to magnetically remove low‐concentrated estrogens from water.
Lukas Müller   +25 more
wiley   +1 more source

Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD System in M31?

open access: yesThe Astrophysical Journal
M31N 2017-01e is the second-fastest recurrent nova known, with a recurrence period of 2.5 yr in the Andromeda galaxy (M31). This system exhibits a unique combination of properties: a low outburst amplitude (∼3 mag), starkly contrasting with known ...
Shatakshi Chamoli   +5 more
doaj   +1 more source

The Narrow Emission Lines of the Very Fast Nova V1721 Aquilae

open access: yesResearch Notes of the AAS
Abstract Infrared spectroscopy, from 12 days after discovery, is presented for the very fast nova V1721 Aquilae. The emission line spectrum, unlike the one present shortly after outburst, is dominated by narrow lines (FWHM ≈ 700 km s −1 ) that include H ...
Richard J. Rudy   +3 more
openaire   +1 more source

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