Laboratory Observation of C and O Emission Lines of the White Dwarf H1504+65-like Atmosphere Model Article Swipe
Bubo Ma
,
Jieru Ren
,
Shaoyi Wang
,
D. H. H. Hoffmann
,
Zhigang Deng
,
Qi Wei
,
Xing Wang
,
Shuai Yin
,
Jianhua Feng
,
Quanping Fan
,
Wei Liu
,
Zhong-Feng Xu
,
Yong Chen
,
Bo Cui
,
Shukai He
,
Zhurong Cao
,
Zongqing Zhao
,
Yuqiu Gu
,
Shaoping Zhu
,
Rui Cheng
,
Xianming Zhou
,
Guoqing Xiao
,
Hongwei Zhao
,
Yihang Zhang
,
Zhe Zhang
,
Yutong Li
,
X. Xu
,
Wenqing Wei
,
Benzheng Chen
,
Shizheng Zhang
,
Zhongmin Hu
,
Lirong Liu
,
Fangfang Li
,
Hao Xu
,
Weimin Zhou
,
Leifeng Cao
,
Yongtao Zhao
·
YOU?
·
· 2021
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ac18c3
YOU?
·
· 2021
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ac18c3
White dwarfs play important roles in stellar evolution and help us gauge the age of our galaxy. The white dwarf H1504+65, the hottest known post-asymptotic giant branch star, is peculiar due to its C- and O-rich but He- and H- deficient atmosphere whose composition cannot be well predicted by current stellar evolution models. The analysis of the elemental abundance and the benchmark of stellar atmospheric models depends heavily on spectral data under cosmic conditions, which are currently extremely scarce. We created a well-defined, uniform, relatively large-scale ∼millimeter plasma sample in the laboratory with a temperature and a C/O ratio similar to those of H1504+65’s atmosphere. The emission spectra with high precision in the range of 10–80 nm were obtained and identified according to databases such as NIST and Kelly. A detailed comparison between our emission lines and the Chandra-observed white dwarf H1504+65 atmosphere’s absorption lines was performed. The stongly isolated O VI lines in the range of 10–13 nm are observed in both cases. We observed a wealth of O V lines in the range of 13–14 nm that cannot be well identified or predicted by models due to the weak flux and also probably due to the blending effect of Fe group elements in the Chandra spectrum. Long-wavelength lines ranging from 14 to 80 nm, which are not observed in the Chandra spectrum because of the high interstellar neutral hydrogen column density, show abundant O IV-V, C IV lines, and strong O VI lines. Moreover, the intensities of the lines at 62.973 and 17.216 nm are analyzed to characterize the plasma temperature.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ac18c3
- https://iopscience.iop.org/article/10.3847/1538-4357/ac18c3/pdf
- OA Status
- bronze
- Cited By
- 10
- References
- 29
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W3208570824
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Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W3208570824Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.3847/1538-4357/ac18c3Digital Object Identifier
- Title
-
Laboratory Observation of C and O Emission Lines of the White Dwarf H1504+65-like Atmosphere ModelWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2021Year of publication
- Publication date
-
2021-10-01Full publication date if available
- Authors
-
Bubo Ma, Jieru Ren, Shaoyi Wang, D. H. H. Hoffmann, Zhigang Deng, Qi Wei, Xing Wang, Shuai Yin, Jianhua Feng, Quanping Fan, Wei Liu, Zhong-Feng Xu, Yong Chen, Bo Cui, Shukai He, Zhurong Cao, Zongqing Zhao, Yuqiu Gu, Shaoping Zhu, Rui Cheng, Xianming Zhou, Guoqing Xiao, Hongwei Zhao, Yihang Zhang, Zhe Zhang, Yutong Li, X. Xu, Wenqing Wei, Benzheng Chen, Shizheng Zhang, Zhongmin Hu, Lirong Liu, Fangfang Li, Hao Xu, Weimin Zhou, Leifeng Cao, Yongtao ZhaoList of authors in order
- Landing page
-
https://doi.org/10.3847/1538-4357/ac18c3Publisher landing page
- PDF URL
-
https://iopscience.iop.org/article/10.3847/1538-4357/ac18c3/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
-
bronzeOpen access status per OpenAlex
- OA URL
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https://iopscience.iop.org/article/10.3847/1538-4357/ac18c3/pdfDirect OA link when available
- Concepts
-
Physics, Astrophysics, White dwarf, Atmosphere (unit), Spectral line, Stellar atmosphere, Interstellar medium, Galaxy, Emission spectrum, Star formation, Flux (metallurgy), Millimeter, Astronomy, Stars, Thermodynamics, Materials science, MetallurgyTop concepts (fields/topics) attached by OpenAlex
- Cited by
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10Total citation count in OpenAlex
- Citations by year (recent)
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2025: 5, 2024: 2, 2023: 2, 2022: 1Per-year citation counts (last 5 years)
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29Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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