The nova V1369 cen - A short review

Luca Izzo; Massimo Della Valle; Francesca Matteucci; Donatella Romano; Luca Pasquini; Leonardo Vanzi; Andres Jordan; Jose Miguel Fernandez; Paz Bluhm; Rafael Brahm; Nestor Espinoza; Robert Williams

The nova V1369 cen - A short review

Luca Izzo, Massimo Della Valle, Francesca Matteucci, Donatella Romano, Luca Pasquini, Leonardo Vanzi, Andres Jordan, Jose Miguel Fernandez, Paz Bluhm, Rafael Brahm, Nestor Espinoza, Robert Williams

Research output: Contribution to journal › Conference article › peer-review

Abstract

We briefly discuss the spectroscopic evolution of the recent outburst of the classical nova V1369 Cen, and the presence of a narrow absorption line identified as due to the resonance of neutral lithium at 6708 Å. We discuss the consequences for the chemical evolution of lithium in the Galaxy. On December 2^nd 2013 a very bright transient was discovered in the southern sky, in the direction of the Centaurus constellation, reaching in few hours the apparent magnitude of V ≈ 4. The transient was soon confirmed to be a nova [1], and the progenitor star coincides almost with a ∼ 15 magnitude star, which was detected by XMM as an X-ray source [2].

Original language	English
Article number	057
Journal	Proceedings of Science
State	Published - 2015
Externally published	Yes
Event	3rd Conference on Golden Age of Cataclysmic Variables and Related Objects, Golden 2015 - Palermo, Italy Duration: 7 Sep 2015 → 12 Sep 2015

Cite this

@article{148ca58b80494b149e8ed9514c2cca71,

title = "The nova V1369 cen - A short review",

abstract = "We briefly discuss the spectroscopic evolution of the recent outburst of the classical nova V1369 Cen, and the presence of a narrow absorption line identified as due to the resonance of neutral lithium at 6708 {\AA}. We discuss the consequences for the chemical evolution of lithium in the Galaxy. On December 2nd 2013 a very bright transient was discovered in the southern sky, in the direction of the Centaurus constellation, reaching in few hours the apparent magnitude of V ≈ 4. The transient was soon confirmed to be a nova [1], and the progenitor star coincides almost with a ∼ 15 magnitude star, which was detected by XMM as an X-ray source [2].",

author = "Luca Izzo and {Della Valle}, Massimo and Francesca Matteucci and Donatella Romano and Luca Pasquini and Leonardo Vanzi and Andres Jordan and Fernandez, {Jose Miguel} and Paz Bluhm and Rafael Brahm and Nestor Espinoza and Robert Williams",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 3rd Conference on Golden Age of Cataclysmic Variables and Related Objects, Golden 2015 ; Conference date: 07-09-2015 Through 12-09-2015",

year = "2015",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - The nova V1369 cen - A short review

AU - Izzo, Luca

AU - Della Valle, Massimo

AU - Matteucci, Francesca

AU - Romano, Donatella

AU - Pasquini, Luca

AU - Vanzi, Leonardo

AU - Jordan, Andres

AU - Fernandez, Jose Miguel

AU - Bluhm, Paz

AU - Brahm, Rafael

AU - Espinoza, Nestor

AU - Williams, Robert

PY - 2015

Y1 - 2015

N2 - We briefly discuss the spectroscopic evolution of the recent outburst of the classical nova V1369 Cen, and the presence of a narrow absorption line identified as due to the resonance of neutral lithium at 6708 Å. We discuss the consequences for the chemical evolution of lithium in the Galaxy. On December 2nd 2013 a very bright transient was discovered in the southern sky, in the direction of the Centaurus constellation, reaching in few hours the apparent magnitude of V ≈ 4. The transient was soon confirmed to be a nova [1], and the progenitor star coincides almost with a ∼ 15 magnitude star, which was detected by XMM as an X-ray source [2].

AB - We briefly discuss the spectroscopic evolution of the recent outburst of the classical nova V1369 Cen, and the presence of a narrow absorption line identified as due to the resonance of neutral lithium at 6708 Å. We discuss the consequences for the chemical evolution of lithium in the Galaxy. On December 2nd 2013 a very bright transient was discovered in the southern sky, in the direction of the Centaurus constellation, reaching in few hours the apparent magnitude of V ≈ 4. The transient was soon confirmed to be a nova [1], and the progenitor star coincides almost with a ∼ 15 magnitude star, which was detected by XMM as an X-ray source [2].

UR - http://www.scopus.com/inward/record.url?scp=85041098680&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85041098680

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 057

T2 - 3rd Conference on Golden Age of Cataclysmic Variables and Related Objects, Golden 2015

Y2 - 7 September 2015 through 12 September 2015

ER -

The nova V1369 cen - A short review

Abstract

Fingerprint

Cite this