X-ray spectroscopy of the classical nova V458 Vulpeculae with Suzaku. Tsujimoto, M., Takei, D., Drake, J., J., Ness, J., U., & Kitamoto, S. Publications of the Astronomical Society of Japan, 61(SUPPL. 1):S69-S76, Oxford University Press, 1, 2009. ![X-ray spectroscopy of the classical nova V458 Vulpeculae with Suzaku [link]](https://bibbase.org/img/filetypes/link.svg "link")
Website abstract bibtex We conducted a target of opportunity X-ray observation of the classical nova V458 Vulpeculae 88 d after the explosion using the Suzaku satellite. With a ̃ 20 ks exposure, the X-ray Imaging Spectrometer detected X-ray emission significantly harder than typical super-soft source emission. The X-ray spectrum shows Kα lines from N, Ne, Mg, Si, and S, and L-series emission from Fe in highly ionized states. The spectrum can be described by a single-temperature (̃0.64keV) thin thermal plasma model in collisional equilibrium with a hydrogen-equivalent extinction column density of ̃3 × 10 21cm-2, a flux of ̃ 10-12ergs -1cm-2, and a luminosity of ̃6 × 10 34ergs-1 in the 0.3-3.0keV band at an assumed distance of 13 kpc. We found a hint of an enhancement of N and deficiencies of O and Fe relative to other metals. The observed X-ray properties can be interpreted as the emission arising from shocks of ejecta from an ONe-type nova. © 2009 Astronomical Society of Japan.
@article{
title = {X-ray spectroscopy of the classical nova V458 Vulpeculae with Suzaku},
type = {article},
year = {2009},
identifiers = {[object Object]},
keywords = {Individual (Nova Vulpeculae 2007 number 1, V458 Vu,Novae,Stars,X-rays},
pages = {S69-S76},
volume = {61},
websites = {https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.sp1.S69,https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.4.L13},
month = {1},
publisher = {Oxford University Press},
day = {30},
id = {55b42bc5-2c93-3afd-b42b-702f5567694d},
created = {2019-11-05T08:27:54.471Z},
accessed = {2018-01-30},
file_attached = {true},
profile_id = {ec4888e4-cd9f-3ee0-90a1-39a024d1537d},
last_modified = {2022-07-15T21:49:05.110Z},
read = {true},
starred = {false},
authored = {true},
confirmed = {true},
hidden = {false},
citation_key = {tsujimoto09},
source_type = {article},
folder_uuids = {9989056f-58f0-4daf-a99f-4779f0cdd416,5a859072-32ae-4559-8859-863b99a8e32c},
private_publication = {false},
abstract = {We conducted a target of opportunity X-ray observation of the classical nova V458 Vulpeculae 88 d after the explosion using the Suzaku satellite. With a ̃ 20 ks exposure, the X-ray Imaging Spectrometer detected X-ray emission significantly harder than typical super-soft source emission. The X-ray spectrum shows Kα lines from N, Ne, Mg, Si, and S, and L-series emission from Fe in highly ionized states. The spectrum can be described by a single-temperature (̃0.64keV) thin thermal plasma model in collisional equilibrium with a hydrogen-equivalent extinction column density of ̃3 × 10 21cm-2, a flux of ̃ 10-12ergs -1cm-2, and a luminosity of ̃6 × 10 34ergs-1 in the 0.3-3.0keV band at an assumed distance of 13 kpc. We found a hint of an enhancement of N and deficiencies of O and Fe relative to other metals. The observed X-ray properties can be interpreted as the emission arising from shocks of ejecta from an ONe-type nova. © 2009 Astronomical Society of Japan.},
bibtype = {article},
author = {Tsujimoto, Masahiro and Takei, Dai and Drake, Jeremy J. and Ness, Jan Uwe and Kitamoto, Shunji},
journal = {Publications of the Astronomical Society of Japan},
number = {SUPPL. 1}
}
Downloads: 0
{"_id":"o2iHPMErAD2MGsbTs","bibbaseid":"tsujimoto-takei-drake-ness-kitamoto-xrayspectroscopyoftheclassicalnovav458vulpeculaewithsuzaku-2009","author_short":["Tsujimoto, M.","Takei, D.","Drake, J., J.","Ness, J., U.","Kitamoto, S."],"bibdata":{"title":"X-ray spectroscopy of the classical nova V458 Vulpeculae with Suzaku","type":"article","year":"2009","identifiers":"[object Object]","keywords":"Individual (Nova Vulpeculae 2007 number 1, V458 Vu,Novae,Stars,X-rays","pages":"S69-S76","volume":"61","websites":"https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.sp1.S69,https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.4.L13","month":"1","publisher":"Oxford University Press","day":"30","id":"55b42bc5-2c93-3afd-b42b-702f5567694d","created":"2019-11-05T08:27:54.471Z","accessed":"2018-01-30","file_attached":"true","profile_id":"ec4888e4-cd9f-3ee0-90a1-39a024d1537d","last_modified":"2022-07-15T21:49:05.110Z","read":"true","starred":false,"authored":"true","confirmed":"true","hidden":false,"citation_key":"tsujimoto09","source_type":"article","folder_uuids":"9989056f-58f0-4daf-a99f-4779f0cdd416,5a859072-32ae-4559-8859-863b99a8e32c","private_publication":false,"abstract":"We conducted a target of opportunity X-ray observation of the classical nova V458 Vulpeculae 88 d after the explosion using the Suzaku satellite. With a ̃ 20 ks exposure, the X-ray Imaging Spectrometer detected X-ray emission significantly harder than typical super-soft source emission. The X-ray spectrum shows Kα lines from N, Ne, Mg, Si, and S, and L-series emission from Fe in highly ionized states. The spectrum can be described by a single-temperature (̃0.64keV) thin thermal plasma model in collisional equilibrium with a hydrogen-equivalent extinction column density of ̃3 × 10 21cm-2, a flux of ̃ 10-12ergs -1cm-2, and a luminosity of ̃6 × 10 34ergs-1 in the 0.3-3.0keV band at an assumed distance of 13 kpc. We found a hint of an enhancement of N and deficiencies of O and Fe relative to other metals. The observed X-ray properties can be interpreted as the emission arising from shocks of ejecta from an ONe-type nova. © 2009 Astronomical Society of Japan.","bibtype":"article","author":"Tsujimoto, Masahiro and Takei, Dai and Drake, Jeremy J. and Ness, Jan Uwe and Kitamoto, Shunji","journal":"Publications of the Astronomical Society of Japan","number":"SUPPL. 1","bibtex":"@article{\n title = {X-ray spectroscopy of the classical nova V458 Vulpeculae with Suzaku},\n type = {article},\n year = {2009},\n identifiers = {[object Object]},\n keywords = {Individual (Nova Vulpeculae 2007 number 1, V458 Vu,Novae,Stars,X-rays},\n pages = {S69-S76},\n volume = {61},\n websites = {https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.sp1.S69,https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.4.L13},\n month = {1},\n publisher = {Oxford University Press},\n day = {30},\n id = {55b42bc5-2c93-3afd-b42b-702f5567694d},\n created = {2019-11-05T08:27:54.471Z},\n accessed = {2018-01-30},\n file_attached = {true},\n profile_id = {ec4888e4-cd9f-3ee0-90a1-39a024d1537d},\n last_modified = {2022-07-15T21:49:05.110Z},\n read = {true},\n starred = {false},\n authored = {true},\n confirmed = {true},\n hidden = {false},\n citation_key = {tsujimoto09},\n source_type = {article},\n folder_uuids = {9989056f-58f0-4daf-a99f-4779f0cdd416,5a859072-32ae-4559-8859-863b99a8e32c},\n private_publication = {false},\n abstract = {We conducted a target of opportunity X-ray observation of the classical nova V458 Vulpeculae 88 d after the explosion using the Suzaku satellite. With a ̃ 20 ks exposure, the X-ray Imaging Spectrometer detected X-ray emission significantly harder than typical super-soft source emission. The X-ray spectrum shows Kα lines from N, Ne, Mg, Si, and S, and L-series emission from Fe in highly ionized states. The spectrum can be described by a single-temperature (̃0.64keV) thin thermal plasma model in collisional equilibrium with a hydrogen-equivalent extinction column density of ̃3 × 10 21cm-2, a flux of ̃ 10-12ergs -1cm-2, and a luminosity of ̃6 × 10 34ergs-1 in the 0.3-3.0keV band at an assumed distance of 13 kpc. We found a hint of an enhancement of N and deficiencies of O and Fe relative to other metals. The observed X-ray properties can be interpreted as the emission arising from shocks of ejecta from an ONe-type nova. © 2009 Astronomical Society of Japan.},\n bibtype = {article},\n author = {Tsujimoto, Masahiro and Takei, Dai and Drake, Jeremy J. and Ness, Jan Uwe and Kitamoto, Shunji},\n journal = {Publications of the Astronomical Society of Japan},\n number = {SUPPL. 1}\n}","author_short":["Tsujimoto, M.","Takei, D.","Drake, J., J.","Ness, J., U.","Kitamoto, S."],"urls":{"Website":"https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.sp1.S69,https://academic.oup.com/pasj/article-lookup/doi/10.1093/pasj/61.4.L13"},"biburl":"https://bibbase.org/service/mendeley/ec4888e4-cd9f-3ee0-90a1-39a024d1537d","bibbaseid":"tsujimoto-takei-drake-ness-kitamoto-xrayspectroscopyoftheclassicalnovav458vulpeculaewithsuzaku-2009","role":"author","keyword":["Individual (Nova Vulpeculae 2007 number 1","V458 Vu","Novae","Stars","X-rays"],"metadata":{"authorlinks":{}},"html":""},"bibtype":"article","biburl":"https://bibbase.org/service/mendeley/ec4888e4-cd9f-3ee0-90a1-39a024d1537d","dataSources":["RmgzPftd92tGag9se","ya2CyA73rpZseyrZ8"],"keywords":["individual (nova vulpeculae 2007 number 1","v458 vu","novae","stars","x-rays"],"search_terms":["ray","spectroscopy","classical","nova","v458","vulpeculae","suzaku","tsujimoto","takei","drake","ness","kitamoto"],"title":"X-ray spectroscopy of the classical nova V458 Vulpeculae with Suzaku","year":2009}