Difference between revisions of "Report On The Discovery Of Interstellar Dust Filaments"
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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 11:01, 1 January 2017
| 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 |
| Journal | None |
| 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.
