Results 91 to 100 of about 77,144 (213)
Observational data on Galactic supernova remnants: II. The supernova remnants within l = 90°-270° [PDF]
Serbian Astronomical Journal, 2004 We have collected all the available data on Galactic supernova remnants given in the literature. The data of Galactic supernova remnants located in the Galactic longitude interval l=90° - 270° in all spectral bands are represented in this work.
Guseinov O.H., Ankayand A., Tagieva S.O.
doaj +1 more source
Logarithmic and Strong Coupling Models in Weyl‐Type f(Q,T)$f(Q,T)$ Gravity
Annalen der Physik, Volume 538, Issue 1, January 2026.This work explores Weyl‐type f(Q,T) gravity using recent observational datasets — CC, Pantheon+, Union 3.0, and DESI DR2. Through MCMC analysis of logarithmic and strong coupling models, the study reveals a transition from deceleration to acceleration, quintessence‐to‐phantom dynamics, and late‐time consistency with LCDM, offering a geometry‐driven ...
Rahul Bhagat, S. K. Tripathy, B. Mishra
wiley +1 more source
SN 2023ixf: The Closest Supernova of the Decade
UniverseSupernova 2023ixf occurred on 18 May 2023 in the nearby galaxy Messier 101 (D≈6.85 Mpc), making it the closest supernova in the last decade. Following its discovery, astronomers around the world rushed to observe the explosion across the electromagnetic ...
Wynn Jacobson-Galán
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Observational data on galactic supernova remnants: I. The supernova remnants within l = 0◦ - 90◦ [PDF]
Serbian Astronomical Journal, 2003 We have collected all the available data on Galactic supernova remnants given in the literature. The data on Galactic supernova remnants located in the Galactic longitude interval l=0◦-90◦ in all the spectral bands are presented in this work.
Guseinov O.H., Ankaj A., Tagieva S.O.
doaj +1 more source
Efficient method for estimating the time evolution of the proto-neutron star mass and radius from a supernova neutrino signal [PDF]
, 2022 Hiroki Nagakura, David Vartanyan
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Quark deconfinement as a supernova explosion engine for massive blue supergiant stars [PDF]
Nature Astronomy, 2017 Blue supergiant stars develop into core-collapse supernovae—one of the most energetic outbursts in the Universe—when all nuclear burning fuel is exhausted in the stellar core.
T. Fischer +8 more
semanticscholar +1 more source
Reading Research Quarterly, Volume 61, Issue 1, January/February/March 2026.In this paper, The Professional Imaginary of Writing Pedagogy is presented as an ideal. This imaginary brings teacher knowledge about the social imaginary for literacy education into relation with teacher professional knowledge and beliefs about writing, to promote pedagogies and practices for writing that are inclusive, expansive, responsive and ...
Clare Dowdall
wiley +1 more source
International Journal of Modern Physics A, 2005 The origin of cosmic rays (CR) is supposed to be closely connected with supernovae (SNe) which create the conditions favorable for various mechanisms of the CR acceleration to operate effectively. First, modern ideas about the physics of the SN explosion are briefly discussed: the explosive thermonuclear burning in degenerate white dwarfs resulting in
Nadyozhin, D. K., Imshennik, V. S.
openaire +2 more sources
BMC Biology, 2018 Background Photosensitizing fluorescent proteins, which generate reactive oxygen species (ROS) upon light irradiation, are useful for spatiotemporal protein inactivation and cell ablation.
Yemima Dani Riani +3 more
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Luminous Radio Emission from the Superluminous Supernova 2017ens at 3.3 yr after Explosion [PDF]
, 2023 R. Margutti +19 more
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