Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012

Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012

Spectroscopic and photometric monitoring observations of nova Apl 2012 (V1724 Apl) were conducted at Koyama Astronomical Observatory, Fujii-Kurosaki Observatory and Bisei Astronomical Observatory. The nova was initially considered as an outbursting pre-main-sequence young stellar object. Our monitor...

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Main Authors: T. Kajikawa, M. Nagashima, H. Kawakita, A. Arai, Y. Ikeda, M. Isogai, M. Fujii, K. Ayani
Format: Article
Language:English
Published: CTU Central Library 2015-02-01
Series:Acta Polytechnica CTU Proceedings
Online Access:https://ojs.cvut.cz/ojs/index.php/APP/article/view/2906
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spelling doaj-ccb71d8e06574037a9c9c6852276e4502020-11-24T23:02:49ZengCTU Central LibraryActa Polytechnica CTU Proceedings2336-53822015-02-012123824110.14311/APP.2015.02.02382668Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012T. Kajikawa0M. Nagashima1H. Kawakita2A. Arai3Y. Ikeda4M. Isogai5M. Fujii6K. Ayani7Kyoto Sangyo Univearsity / Koyama Astronomical ObservatoryKyoto Sangyo Univearsity / Koyama Astronomical ObservatoryKyoto Sangyo Univearsity / Koyama Astronomical ObservatoryKyoto Sangyo Univearsity / Koyama Astronomical Observatory University of Hyogo / Nishi-Harima Astronomical ObservatoryKyoto Sangyo Univearsity / Koyama Astronomical ObservatoryNational Astronomical Observatory of JapanFujii-Kurosaki ObservatoryBisei Astronomical ObservatorySpectroscopic and photometric monitoring observations of nova Apl 2012 (V1724 Apl) were conducted at Koyama Astronomical Observatory, Fujii-Kurosaki Observatory and Bisei Astronomical Observatory. The nova was initially considered as an outbursting pre-main-sequence young stellar object. Our monitoring observations have revealed the nova to be a Fe II type classical nova. The temporal evolution of spectra and light curves of the nova were similar to those of a slow nova (e.g., V1280 Sco and V5558 Sgr). We observed no evidence of molecule formation in V1724 Aql in contrast with V2676 Oph in which dust formation occurred after the molecular formation in the nova outflow.https://ojs.cvut.cz/ojs/index.php/APP/article/view/2906
collection DOAJ
language English
format Article
sources DOAJ
author T. Kajikawa
M. Nagashima
H. Kawakita
A. Arai
Y. Ikeda
M. Isogai
M. Fujii
K. Ayani
spellingShingle T. Kajikawa
M. Nagashima
H. Kawakita
A. Arai
Y. Ikeda
M. Isogai
M. Fujii
K. Ayani
Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012
Acta Polytechnica CTU Proceedings
author_facet T. Kajikawa
M. Nagashima
H. Kawakita
A. Arai
Y. Ikeda
M. Isogai
M. Fujii
K. Ayani
author_sort T. Kajikawa
title Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012
title_short Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012
title_full Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012
title_fullStr Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012
title_full_unstemmed Spectroscopic Monitoring Observations of Nova V1724 Aql in 2012
title_sort spectroscopic monitoring observations of nova v1724 aql in 2012
publisher CTU Central Library
series Acta Polytechnica CTU Proceedings
issn 2336-5382
publishDate 2015-02-01
description Spectroscopic and photometric monitoring observations of nova Apl 2012 (V1724 Apl) were conducted at Koyama Astronomical Observatory, Fujii-Kurosaki Observatory and Bisei Astronomical Observatory. The nova was initially considered as an outbursting pre-main-sequence young stellar object. Our monitoring observations have revealed the nova to be a Fe II type classical nova. The temporal evolution of spectra and light curves of the nova were similar to those of a slow nova (e.g., V1280 Sco and V5558 Sgr). We observed no evidence of molecule formation in V1724 Aql in contrast with V2676 Oph in which dust formation occurred after the molecular formation in the nova outflow.
url https://ojs.cvut.cz/ojs/index.php/APP/article/view/2906
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AT mnagashima spectroscopicmonitoringobservationsofnovav1724aqlin2012
AT hkawakita spectroscopicmonitoringobservationsofnovav1724aqlin2012
AT aarai spectroscopicmonitoringobservationsofnovav1724aqlin2012
AT yikeda spectroscopicmonitoringobservationsofnovav1724aqlin2012
AT misogai spectroscopicmonitoringobservationsofnovav1724aqlin2012
AT mfujii spectroscopicmonitoringobservationsofnovav1724aqlin2012
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