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1865 Plaskett (3 results)
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![Stock image for Experiments Regarding Efficiency of Spectrographs [microform] for sale by THE SAINT BOOKSTORE](https://pictures.abebooks.com/isbn/9781014022776-us-300.jpg)
Experiments Regarding Efficiency of Spectrographs [microform]
Seller: THE SAINT BOOKSTORE, Southport, United Kingdom
Seller rating 5 out of 5 stars
US$ 23.87
US$ 16.52 shipping
Ships from United Kingdom to U.S.A.Quantity: Over 20 available
Add to basketPaperback / softback. Condition: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.
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![Stock image for The Spectroscopic Binary [Thêta] Tauri [microform] for sale by THE SAINT BOOKSTORE](https://pictures.abebooks.com/isbn/9781015087682-us-300.jpg)
The Spectroscopic Binary [Thêta] Tauri [microform]
Seller: THE SAINT BOOKSTORE, Southport, United Kingdom
Seller rating 5 out of 5 stars
US$ 23.87
US$ 16.52 shipping
Ships from United Kingdom to U.S.A.Quantity: Over 20 available
Add to basketPaperback / softback. Condition: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.
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The structure and rotation of the galaxy.
Published by The American Philosophical Society, 1930., In: Proceedings of the American Philosophical Society held at Philadelphia for Promoting Useful Knowledge, Vol. LXIX, 1930. Phil, 1930
Seller: Jeff Weber Rare Books, Neuchatel, NEUCH, Switzerland
Seller rating 4 out of 5 stars
First Edition
In: Proceedings of the American Philosophical Society held at Philadelphia for Promoting Useful Knowledge, Vol. LXIX, 1930. Philadelphia:: The American Philosophical Society, 1930., 1930. 245 x 170 mm. Thick 8vo. Pages 401-417. [Entire volume: xix, 580 pp.]. 4 tables. Dark green buckram, gilt spine. Ex library blind-stamp of the Carnegie Institution of Washington Mount Wilson Observatory. Fine. FIRST EDITION. "But perhaps his most notable achievement was his application of spectroscopic evidence to the problem of galactic rotation and the distance and direction of the center of gravity of the galaxy, those being determined from the motions of stars of spectral types O5 to B7 (1930)." DSB, XI, pp. 18-19.
