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Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star
We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of...
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Published in: | Publications of the Astronomical Society of the Pacific 1993-06, Vol.105 (688), p.599-602 |
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container_issue | 688 |
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container_title | Publications of the Astronomical Society of the Pacific |
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creator | Kaler, James B. Bell, David Hayes, John Stanghellini, Letizia |
description | We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of a symbiotic star. |
doi_str_mv | 10.1086/133202 |
format | article |
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source | JSTOR Archival Journals and Primary Sources Collection; Institute of Physics |
subjects | Astronomical objects Astronomy Density Earth, ocean, space Exact sciences and technology Helium Interstellar extinction Interstellar medium (ism) and nebulae in milky way Nebulae Nitrogen Planetary nebulae Stars Stellar spectra Stellar systems. Galactic and extragalactic objects and systems. The universe Symbiotic stars |
title | Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star |
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