SOFIA/upGREAT far-infrared spectroscopy of bright rimmed pillars in IC 1848 Article Swipe
D. C. Lis
,
R. Guêsten
,
P. F. Goldsmith
,
Yoko Okada
,
Young Min Seo
,
H. Wiesemeyer
,
Marc Mertens
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202451760
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202451760
Using the upGREAT instrument on SOFIA, we imaged the [C II ] 158 µm fine structure line emission in bright-rimmed pillars located at the southern edge of the IC 1848 H II region, and carried out pointed observations of the [O I ] 63 and 145 µm fine structure lines toward selected positions. The observations are used to characterize the morphology, velocity field, and the physical conditions in the G1–G3 filaments. The velocity-resolved [C II ] spectra show evidence of a velocity shift at the head of the brightest G1 filament, possibly caused by radiation pressure from the impinging UV photons or the rocket effect of the evaporating gas. Archival Herschel PACS and SPIRE observations imply H 2 column densities in the range 10 21 –10 22 cm −2 , corresponding to maximum visual extinction A V ≃ 10 mag, and average H 2 volume density of ≃4500 cm −3 in the filaments. The [C II ] emission traces ∼17% of the total H 2 column density, as derived from dust SED fits. Photon-dominated region models are unable to explain the observed line intensities of the two [O I ] fine structure lines in IC 1848, with the observed [O I ] 145 µm line being too strong compared to the model predictions. The [O I ] lines in IC 1848 are overall weak and the signal-to-noise ratio is limited. However, our observations suggest that the [O I ] 63/145 µm intensity ratio is a sensitive probe of the physical conditions in photon-dominated regions such as IC 1848. These lines are thus excellent targets for future high-altitude balloon instruments, less affected by telluric absorption.
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- Type
- article
- Language
- en
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- https://doi.org/10.1051/0004-6361/202451760
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https://openalex.org/W4402976496Canonical identifier for this work in OpenAlex
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https://doi.org/10.1051/0004-6361/202451760Digital Object Identifier
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SOFIA/upGREAT far-infrared spectroscopy of bright rimmed pillars in IC 1848Work title
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articleOpenAlex work type
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enPrimary language
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2024Year of publication
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2024-09-30Full publication date if available
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D. C. Lis, R. Guêsten, P. F. Goldsmith, Yoko Okada, Young Min Seo, H. Wiesemeyer, Marc MertensList of authors in order
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https://doi.org/10.1051/0004-6361/202451760Publisher landing page
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hybridOpen access status per OpenAlex
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https://doi.org/10.1051/0004-6361/202451760Direct OA link when available
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Physics, Astrophysics, Spectroscopy, Infrared, Astronomy, Far infrared, Infrared spectroscopy, Near-infrared spectroscopy, Optics, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
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1Total citation count in OpenAlex
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| abstract_inverted_index.model | 211 |
| abstract_inverted_index.probe | 246 |
| abstract_inverted_index.range | 122 |
| abstract_inverted_index.ratio | 227, 242 |
| abstract_inverted_index.shift | 82 |
| abstract_inverted_index.total | 162 |
| abstract_inverted_index.–10 | 125 |
| abstract_inverted_index.63/145 | 239 |
| abstract_inverted_index.SOFIA, | 5 |
| abstract_inverted_index.caused | 92 |
| abstract_inverted_index.column | 118, 165 |
| abstract_inverted_index.effect | 104 |
| abstract_inverted_index.field, | 62 |
| abstract_inverted_index.future | 265 |
| abstract_inverted_index.imaged | 7 |
| abstract_inverted_index.models | 175 |
| abstract_inverted_index.region | 174 |
| abstract_inverted_index.rocket | 103 |
| abstract_inverted_index.strong | 207 |
| abstract_inverted_index.toward | 50 |
| abstract_inverted_index.traces | 158 |
| abstract_inverted_index.unable | 177 |
| abstract_inverted_index.visual | 133 |
| abstract_inverted_index.volume | 144 |
| abstract_inverted_index.∼17% | 159 |
| abstract_inverted_index.G1–G3 | 69 |
| abstract_inverted_index.average | 141 |
| abstract_inverted_index.balloon | 267 |
| abstract_inverted_index.carried | 34 |
| abstract_inverted_index.density | 145 |
| abstract_inverted_index.derived | 168 |
| abstract_inverted_index.explain | 179 |
| abstract_inverted_index.located | 21 |
| abstract_inverted_index.maximum | 132 |
| abstract_inverted_index.overall | 222 |
| abstract_inverted_index.photons | 100 |
| abstract_inverted_index.pillars | 20 |
| abstract_inverted_index.pointed | 36 |
| abstract_inverted_index.region, | 32 |
| abstract_inverted_index.regions | 253 |
| abstract_inverted_index.spectra | 76 |
| abstract_inverted_index.suggest | 233 |
| abstract_inverted_index.targets | 263 |
| abstract_inverted_index.upGREAT | 2 |
| abstract_inverted_index.≃4500 | 147 |
| abstract_inverted_index.Archival | 109 |
| abstract_inverted_index.Herschel | 110 |
| abstract_inverted_index.However, | 230 |
| abstract_inverted_index.affected | 270 |
| abstract_inverted_index.compared | 208 |
| abstract_inverted_index.density, | 166 |
| abstract_inverted_index.emission | 17, 157 |
| abstract_inverted_index.evidence | 78 |
| abstract_inverted_index.limited. | 229 |
| abstract_inverted_index.observed | 181, 198 |
| abstract_inverted_index.physical | 65, 249 |
| abstract_inverted_index.possibly | 91 |
| abstract_inverted_index.pressure | 95 |
| abstract_inverted_index.selected | 51 |
| abstract_inverted_index.southern | 24 |
| abstract_inverted_index.telluric | 272 |
| abstract_inverted_index.velocity | 61, 81 |
| abstract_inverted_index.brightest | 88 |
| abstract_inverted_index.densities | 119 |
| abstract_inverted_index.excellent | 262 |
| abstract_inverted_index.filament, | 90 |
| abstract_inverted_index.impinging | 98 |
| abstract_inverted_index.intensity | 241 |
| abstract_inverted_index.radiation | 94 |
| abstract_inverted_index.sensitive | 245 |
| abstract_inverted_index.structure | 15, 48, 191 |
| abstract_inverted_index.conditions | 66, 250 |
| abstract_inverted_index.extinction | 134 |
| abstract_inverted_index.filaments. | 70, 152 |
| abstract_inverted_index.instrument | 3 |
| abstract_inverted_index.positions. | 52 |
| abstract_inverted_index.absorption. | 273 |
| abstract_inverted_index.evaporating | 107 |
| abstract_inverted_index.intensities | 183 |
| abstract_inverted_index.morphology, | 60 |
| abstract_inverted_index.characterize | 58 |
| abstract_inverted_index.instruments, | 268 |
| abstract_inverted_index.observations | 37, 54, 114, 232 |
| abstract_inverted_index.predictions. | 212 |
| abstract_inverted_index.bright-rimmed | 19 |
| abstract_inverted_index.corresponding | 130 |
| abstract_inverted_index.high-altitude | 266 |
| abstract_inverted_index.signal-to-noise | 226 |
| abstract_inverted_index.Photon-dominated | 173 |
| abstract_inverted_index.photon-dominated | 252 |
| abstract_inverted_index.velocity-resolved | 72 |
| cited_by_percentile_year.max | 95 |
| cited_by_percentile_year.min | 91 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 7 |
| citation_normalized_percentile.value | 0.78042715 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |