Classical novae with CUBES
Among the main science cases that have motivated the proposal of CUBES, a new high-resolution spectrograph for the Very Large Telescope at the European Southern Observatory, there is the study and the characterisation of the nucleosynthesis of beryllium. Classical novae have been proposed since the...
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| Veröffentlicht in: | Experimental Astronomy 2023-02, Vol.55 (1), p.191-198 |
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| creator | Izzo, Luca Molaro, Paolo Bonifacio, Piercarlo Cescutti, Gabriele Della Valle, Massimo Selvelli, Pierluigi |
| description | Among the main science cases that have motivated the proposal of CUBES, a new high-resolution spectrograph for the Very Large Telescope at the European Southern Observatory, there is the study and the characterisation of the nucleosynthesis of beryllium. Classical novae have been proposed since the ’70s as one of the main factories of lithium in the Galaxy, but this hypothesis has been demonstrated on empirical basis only recently thanks to the direct identification of lithium in V1369 Cen and through the observations of the resonance transition of
7
Be II, the
7
Li parent, at 313.0 nm in the near-UV range. CUBES is then the ideal instrument to quantify the amount of
7
Be and therefore of
7
Li produced by the different novae types hosted in the different components of the Milky Way and also in its nearby satellite galaxies. As important by-product of high resolution spectroscopic observations obtained with CUBES, there are the study of the properties of nova ejecta abundances, the shocks evolution in novae and their connection with the high-energy emission observed in these transients, from satellites as Fermi and Swift. |
| doi_str_mv | 10.1007/s10686-022-09876-3 |
| format | Article |
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7
Be II, the
7
Li parent, at 313.0 nm in the near-UV range. CUBES is then the ideal instrument to quantify the amount of
7
Be and therefore of
7
Li produced by the different novae types hosted in the different components of the Milky Way and also in its nearby satellite galaxies. As important by-product of high resolution spectroscopic observations obtained with CUBES, there are the study of the properties of nova ejecta abundances, the shocks evolution in novae and their connection with the high-energy emission observed in these transients, from satellites as Fermi and Swift.</description><identifier>ISSN: 0922-6435</identifier><identifier>EISSN: 1572-9508</identifier><identifier>DOI: 10.1007/s10686-022-09876-3</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astronomy ; Beryllium ; Beryllium 7 ; Chemistry and Earth Sciences ; Computer Science ; Cubes ; Ejecta ; European Southern Observatory ; Galaxies ; High energy astronomy ; High resolution ; Lithium isotopes ; Novae ; Nuclear fusion ; Observations and Techniques ; Original Article ; Physics ; Physics and Astronomy ; Satellites ; Sciences of the Universe ; Statistics for Engineering ; Very Large Telescope</subject><ispartof>Experimental Astronomy, 2023-02, Vol.55 (1), p.191-198</ispartof><rights>The Author(s), under exclusive licence to Springer Nature B.V. 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c305t-e9a5c5b864df5b0b00b40532d31f6719b4f37c7d473a6f29e2f464644af2b36e3</cites><orcidid>0000-0001-9695-8472</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10686-022-09876-3$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10686-022-09876-3$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,777,781,882,27905,27906,41469,42538,51300</link.rule.ids><backlink>$$Uhttps://insu.hal.science/insu-03849370$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Izzo, Luca</creatorcontrib><creatorcontrib>Molaro, Paolo</creatorcontrib><creatorcontrib>Bonifacio, Piercarlo</creatorcontrib><creatorcontrib>Cescutti, Gabriele</creatorcontrib><creatorcontrib>Della Valle, Massimo</creatorcontrib><creatorcontrib>Selvelli, Pierluigi</creatorcontrib><title>Classical novae with CUBES</title><title>Experimental Astronomy</title><addtitle>Exp Astron</addtitle><description>Among the main science cases that have motivated the proposal of CUBES, a new high-resolution spectrograph for the Very Large Telescope at the European Southern Observatory, there is the study and the characterisation of the nucleosynthesis of beryllium. Classical novae have been proposed since the ’70s as one of the main factories of lithium in the Galaxy, but this hypothesis has been demonstrated on empirical basis only recently thanks to the direct identification of lithium in V1369 Cen and through the observations of the resonance transition of
7
Be II, the
7
Li parent, at 313.0 nm in the near-UV range. CUBES is then the ideal instrument to quantify the amount of
7
Be and therefore of
7
Li produced by the different novae types hosted in the different components of the Milky Way and also in its nearby satellite galaxies. 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Classical novae have been proposed since the ’70s as one of the main factories of lithium in the Galaxy, but this hypothesis has been demonstrated on empirical basis only recently thanks to the direct identification of lithium in V1369 Cen and through the observations of the resonance transition of
7
Be II, the
7
Li parent, at 313.0 nm in the near-UV range. CUBES is then the ideal instrument to quantify the amount of
7
Be and therefore of
7
Li produced by the different novae types hosted in the different components of the Milky Way and also in its nearby satellite galaxies. As important by-product of high resolution spectroscopic observations obtained with CUBES, there are the study of the properties of nova ejecta abundances, the shocks evolution in novae and their connection with the high-energy emission observed in these transients, from satellites as Fermi and Swift.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s10686-022-09876-3</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0001-9695-8472</orcidid><oa>free_for_read</oa></addata></record> |
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| subjects | Astronomy Beryllium Beryllium 7 Chemistry and Earth Sciences Computer Science Cubes Ejecta European Southern Observatory Galaxies High energy astronomy High resolution Lithium isotopes Novae Nuclear fusion Observations and Techniques Original Article Physics Physics and Astronomy Satellites Sciences of the Universe Statistics for Engineering Very Large Telescope |
| title | Classical novae with CUBES |
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