Citation
Willner, Steven Paul (1976) Compact Infrared Sources: NGC 7538 and the Galactic Center. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/YGRP-NJ17. https://resolver.caltech.edu/CaltechETD:etd-08252008-153611
Abstract
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in .pdf document. Three infrared and radio sources in NGC 7538 have been observed from 8 to 13 [...] with 1% spectral and 5" spatial resolution. The very small southern source shows a deep silicate absorption feature at 9.7 [...] while the northern extended source shows little or no silicate absorption, but has a 12.8-[...] emission line from Ne II. The data imply that the compact source has a gas to dust ratio of 75 inside the ionized region. The extended source only 10" away has a gas to dust ratio implied by the 10-[...] data alone of 3 x 10[...], but the true ratio must be much lower to account for published 20-[...] measurements. A revised 10-[...] map of the Galactic center with 2[...]3 resolution, broadband photometry of individual sources from 1.2 to 20 [...], and 8 to 13-[...] photometry of individual sources with 1% spectral resolution have been obtained. The principal conclusions of this study are: (1) The five sources with the bluest energy distributions between 1.6 and 3.5 [...] are stars or star clusters. The brightest has a luminosity of 10[...] L[...] while the other four have luminosities of about 10[...] L[...]. (2) There is extended emission from ionized gas and dust. (3) The density of ionized gas in the discrete 10-[...] sources is no higher than that in the extended source. (4) There is at least one compact source that is not associated with the others and has a different energy distribution. (5) Most of the extinction toward the sources observed is interstellar and is moderately uniform. The visual extinction is about 28 magnitudes, and the 9.7-[...] silicate extinction is about 3.7 magnitudes.
Item Type: | Thesis (Dissertation (Ph.D.)) |
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Subject Keywords: | (Astronomy) |
Degree Grantor: | California Institute of Technology |
Division: | Physics, Mathematics and Astronomy |
Major Option: | Astronomy |
Thesis Availability: | Public (worldwide access) |
Research Advisor(s): |
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Group: | Astronomy Department |
Thesis Committee: |
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Defense Date: | 29 January 1976 |
Record Number: | CaltechETD:etd-08252008-153611 |
Persistent URL: | https://resolver.caltech.edu/CaltechETD:etd-08252008-153611 |
DOI: | 10.7907/YGRP-NJ17 |
Default Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
ID Code: | 3225 |
Collection: | CaltechTHESIS |
Deposited By: | Imported from ETD-db |
Deposited On: | 09 Sep 2008 |
Last Modified: | 16 Aug 2024 22:48 |
Thesis Files
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PDF (Willner_sp_1976.pdf)
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