Velocity-resolved [ ] Emission from Cold Diffuse Clouds in the Interstellar Medium Article Swipe
P. F. Goldsmith
,
J. L. Pineda
,
David A. Neufeld
,
M. G. Wolfire
,
C. Risacher
,
R. Simon
·
YOU?
·
· 2018
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/aab34e
YOU?
·
· 2018
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/aab34e
We have combined emission from the 158 μ m fine structure transition of C + observed with the GREAT and upGREAT instruments on SOFIA with 21 cm absorption spectra and visual extinction to characterize the diffuse interstellar clouds found along the lines of sight. The weak [C ii ] emission is consistent in velocity and line width with the strongest H i component produced by the cold neutral medium. The H i column density and kinetic temperature are known from the 21 cm data and, assuming a fractional abundance of ionized carbon, we calculate the volume density and thermal pressure of each source, which vary considerably, with 27 cm −3 considering only the atomic hydrogen along the lines of sight to be responsible for the C + , while 13 cm −3 including the hydrogen in both forms. The thermal pressure varies widely with 1970 cm −3 K 10,440 cm −3 K for H 0 alone and 750 cm −3 K ≤ P th / k ≤ 9360 cm −3 K including both H 0 and H 2 . The molecular hydrogen fraction varies between 0.10 and 0.67. Photoelectric heating is the dominant heating source, supplemented by a moderately enhanced cosmic ray ionization rate, constrained by the relatively low 45 K to 73 K gas temperatures of the clouds. The resulting thermal balance for the two lower-density clouds is satisfactory, but for the two higher-density clouds, the combined heating rate is insufficient to balance the observed C + cooling.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/aab34e
- https://iopscience.iop.org/article/10.3847/1538-4357/aab34e/pdf
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- Cited By
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- References
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https://doi.org/10.3847/1538-4357/aab34eDigital Object Identifier
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Velocity-resolved [ ] Emission from Cold Diffuse Clouds in the Interstellar MediumWork title
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articleOpenAlex work type
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enPrimary language
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2018Year of publication
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2018-03-28Full publication date if available
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P. F. Goldsmith, J. L. Pineda, David A. Neufeld, M. G. Wolfire, C. Risacher, R. SimonList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4357/aab34ePublisher landing page
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https://iopscience.iop.org/article/10.3847/1538-4357/aab34e/pdfDirect link to full text PDF
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bronzeOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/1538-4357/aab34e/pdfDirect OA link when available
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2025: 2, 2024: 1, 2023: 3, 2022: 1, 2021: 4Per-year citation counts (last 5 years)
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47Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| primary_location.landing_page_url | https://doi.org/10.3847/1538-4357/aab34e |
| publication_date | 2018-03-28 |
| publication_year | 2018 |
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