Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Ivan De Gennaro Aquino"'
Publikováno v:
Astronomy & Astrophysics. 639:L12
Context. Extreme super-solar abundances of lithium and beryllium have been reported in recent years for classical novae based on absorption lines in ultraviolet and optical spectra during the optically thick stages, but these findings have not been c
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f329a7474c222083ddd3043ac70cd0f
https://doi.org/10.1051/0004-6361/202038599
https://doi.org/10.1051/0004-6361/202038599
A fraction of classical novae form dust during the early stages of their outbursts. The classical CO nova V5668 Sgr (Nova Sgr. 2015b) underwent a deep photometric minimum about 100 days after outburst that was covered across the spectrum. A similar e
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6d28917dc9540ee1a3b770ffef03961
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Nova Cen 2013 (V1369 Cen) is the fourth bright nova observed panchromatically through high-resolution UV+optical multiepoch spectroscopy. It is also the nova with the richest set of spectra (in terms of both data quality and number of epochs) thanks
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5dbebef97d09e9f4dbbbf890a774550
http://hdl.handle.net/11568/1023338
http://hdl.handle.net/11568/1023338
We critically examine the recent claimed detection of Raman scattered O VI at around 6830\AA\ in the iron curtain stage spectra of the classical CO nova V339 Del. The observed line variations are compatible in profile and timing of emission line stre
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78029491c5524866057a42d93f676ccf