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HI Study of Southern Galactic Supernova Remnants
Astrophysics · Submitted 6 Nov 2003
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results.
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The abstract, sentence by sentence
We briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. | contribution 0.93 | 0.80 | 0.07 | asserted 0.65 |
| s1 | For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results. | contribution 0.55 | 0.77 | 0.10 | unclear 0.69 |
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The paper
Original abstract
We briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results.
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