Egan, M. P.; Clark, J. S.; Mizuno, D. R.; Carey, S. J.; Steele, I. A. and Price, S. D.
|DOI (Digital Object Identifier) Link:||http://doi.org/10.1086/340222|
|Google Scholar:||Look up in Google Scholar|
The Midcourse Space Experiment (MSX) Galactic plane survey discovered a nearly perfectly circular ring nebula around the suspected planetary nebula Wray 17-96. Using near-IR spectral typing and modeling of the mid-IR nebula, we find that Wray 17-96 is more likely a candidate to be a luminous blue variable (LBV) surrounded by a large spherical ejecta shell. It is very similar to the G79.29+0.46 LBV candidate in Cygnus and the Pistol Star. The K-band spectrum and the mid-IR data indicate a stellar temperature of 13,000 K. The most likely distance to the source is 4.5 kpc, leading to a luminosity of 1.8 × 106 L. We suggest that the nebula consists of multiple shells and that an evolution from oxygen-rich to carbon-rich chemistry may be indicated.
|Item Type:||Journal Article|
|Keywords:||infrared: stars; planetary nebulae: individual (Wray 17-96); stars: evolution; stars: variables: other|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||17 Feb 2009 09:55|
|Last Modified:||04 Oct 2016 10:18|
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