83. Truth and Satisfaction: The Gist of Pragmaticism

Proceedings of Accretion Processes in Cosmic Sources – II — PoS(APCS2018)

2019

Section: Pos(apcs2018)057mentioning

confidence: 99%

Galactic and Extragalactic Novae - A Review

Proceedings of Accretion Processes in Cosmic Sources – II — PoS(APCS2018)

2019

“…I am monitoring novae (mostly Northern) since 2005 at the Cassini 1.5m telescope equipped with the BFOSC Imager/Spectrograph [89]. Optical spectra are secured during the decline to monitor the evolution of the novae, with the highest possible cadence.…”

Section: Spectroscopic Evolutionmentioning

confidence: 99%

Galactic and extragalactic novae - A Review

Proceedings of Accretion Processes in Cosmic Sources — PoS(APCS2016)

2018

The outbursts of classical novae are among the strongest explosions in the Universe. The multifrequency observations are contributing to understanding the process of explosions and of the long term evolution. In this review, I discuss the observations of novae over the electromagnetic spectrum, focusing on the morphology of the decline light curves, the spectroscopic investigations, the long term evolution, the recurrent novae, the gamma ray emission in novae, extragalactic novae and the gravitational emission of novae.

“…Since 2005 I am monitoring Northern novae at the Cassini 1.5m telescope, using the BFOSC Imager/Spectrograph [111]. Optical spectra are secured during the decline with the densest possible sampling.…”

Section: Spectroscopic Evolutionmentioning

confidence: 99%

Multifrequency Behaviour of Galactic and Extragalactic Novae

Proceedings of XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop — PoS(MULTIF2017)

2018

The outbursts of novae are among the strongest explosions in the Universe. The eruptions involve physical processes that span the whole electromagnetic spectrum, demanding multifrequency observations. The photometric and spectroscopic observations in the optical domain are combined with radio, infrared, X-ray and gamma ray observations, allowing to discover new phenomena, like the GeV gamma ray emission.