Report On The Discovery Of Interstellar Dust Filaments: Difference between revisions
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| keywords = [[Dust]], [[Gas]], [[Interstellar Medium]] | | keywords = [[Dust]], [[Gas]], [[Interstellar Medium]] | ||
| published = 1977 | | published = 1977 | ||
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Observational evidence described reveals the presence of previously unrecognized interstellar dust filaments against the luminous backgrounds provided by: Milky Way starfields, globular clusters, galaxies, supernova remnants, galactic clusters, HII regions, reflection nebulae, and planetary nebulae. | Observational evidence described reveals the presence of previously unrecognized interstellar dust filaments against the luminous backgrounds provided by: Milky Way starfields, globular clusters, galaxies, supernova remnants, galactic clusters, HII regions, reflection nebulae, and planetary nebulae. | ||
[[Category:Scientific Paper]] | [[Category:Scientific Paper|report discovery interstellar dust filaments]] | ||
Latest revision as of 19:31, 18 July 2026
| Scientific Paper | |
|---|---|
| Title | Report On The Discovery Of Interstellar Dust Filaments |
| Read in full | Link to paper |
| Author(s) | Harry Hamlin Ricker |
| Keywords | Dust, Gas, Interstellar Medium |
| Published | 1977 |
| No. of pages | 17 |
Read the full paper here
Abstract
Observational evidence described reveals the presence of previously unrecognized interstellar dust filaments against the luminous backgrounds provided by: Milky Way starfields, globular clusters, galaxies, supernova remnants, galactic clusters, HII regions, reflection nebulae, and planetary nebulae.