Results 91 to 100 of about 85,351 (144)
Molecular Oncology, Volume 20, Issue S1, Page 1-692, August 2026.Abstracts submitted to the ‘EACR 2026 Congress: Innovative Cancer Science’, from 08–11 June 2026 and accepted by the Congress Organising Committee are published in this Supplement of Molecular Oncology, an affiliated journal of the European Association for Cancer Research (EACR).
wiley +1 more source
Very high energy gamma-ray follow-up observations of novae and dwarf novae with the MAGIC telescopes [PDF]
, 2015 In the last few years the Fermi-LAT instrument has detected GeV gamma-ray emission from several novae. Such GeV emission can be interpreted in terms of inverse Compton emission from electrons accelerated in the shock or in terms of emission from hadrons ...
Sitarek J. +7 more
core +1 more source
The symbiotic recurrent nova V745 Sco at radio wavelengths
Monthly Notices of the Royal Astronomical SocietyABSTRACT V745 Sco is a Galactic symbiotic recurrent nova with nova eruptions in 1937, 1989, and 2014. We study the behaviour of V745 Sco at radio wavelengths (0.6–37 GHz), covering both its 1989 and 2014 eruptions and informed by optical, X-ray, and $\gamma$-ray data. The radio light curves are synchrotron-dominated.
Isabella Molina +16 more
openaire +2 more sources
Outbursts in Symbiotic Binaries: Z and Continued Observation [PDF]
, 2005 A major question for symbiotic stars concerns the nature and cause of their outbursts. A small subset of symbiotics, the "slow novae" are fairly well established as thermonuclear events that last on the order of decades.
Sonneborn, George, Keyes, Charles
core
Astronomy & AstrophysicsIn this paper, we present a description and characterisation of the 2-Channel Focal Reducer Rozhen (FoReRo2), with an emphasis on its polarimetric and spectropolarimetric observation modes.
Nikolov Yanko +5 more
doaj +1 more source
Open Astronomy, 2012 We have analyzed the optical light curve of the symbiotic star V407 Cyg that underwent a classical nova outburst in 2010 March. Being guided by a supersoft X-ray phase observed during days 20-40 after the nova outburst, we are able to reproduce the light
Hachisu I., Kato M.
doaj +1 more source
, 2018 L'association Artes Novae organise une visite de l'exposition « Naissance de la sculpture gothique. Saint-Denis, Paris, Chartres, 1135-1150 » (10 octobre 2018-21 janvier 2019) conduite par Philippe Plagnieux, professeur en histoire de l'art médiéval ...
Artes Novae
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The First Hours and Days of the 2021 Explosion of the Recurrent Symbiotic Nova RS Ophiuchii
The Astrophysical JournalThe accretion of matter onto a massive white dwarf (WD) can lead to repeated nuclear explosions on its surface over a timescale of years to decades. The seventh explosion of the recurrent symbiotic nova RS Ophiuchi (RS Oph) was recorded on 2021 August 8.
Augustin Skopal +6 more
doaj +1 more source
Multiwavelength Timing Analysis of the Recurrent Nova T CrB
UniverseWe present a short-timescale multiwavelength timing study of the symbiotic recurrent nova T Coronae Borealis (T CrB), based on Swift/X-Ray Telescope (XRT), Swift/UltraViolet Optical Telescope (UVOT), and Transiting Exoplanet Survey Satellite (TESS ...
Xiaowan Zhang +3 more
doaj +1 more source
The Role of Binary Configuration in Shaping Nova Evolution via Wind Accretion in Symbiotic Systems
The Astrophysical JournalWe investigate the impact of the Bondi–Hoyle–Lyttleton (BHL) accretion mechanism on the evolution of nova eruptions in symbiotic systems by systematically varying three key input parameters: the initial donor (asymptotic giant branch, AGB) mass, the ...
Irin Babu Vathachira +2 more
doaj +1 more source