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The Carbon Star Phenomenon. Proceedings of the 77th Symposium of the International Astronomical Union, Held in Antalya, Turkey, May 27-31,1996. Proceedings of the 177th Symposiumn of the International Astronomical Union, Held in Antalya, Turkey, May 27-3
Robert F. . Ed(S): Wing
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Description for The Carbon Star Phenomenon. Proceedings of the 77th Symposium of the International Astronomical Union, Held in Antalya, Turkey, May 27-31,1996. Proceedings of the 177th Symposiumn of the International Astronomical Union, Held in Antalya, Turkey, May 27-3
Hardback. Proceedings of the 177th Symposium of the International Astronomical Union, held in Antalya, Turkey, May 27-31, 1996 Editor(s): Wing, Robert F. Series: International Astronomical Union Symposia (Closed). Num Pages: 654 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 34. Weight in Grams: 1089.
The atmospheres of many stars have chemical compositions that are significantly different from that of the interstellar medium from which they are formed. This symposium considered all kinds of late-type stars showing altered compositions, the carbon stars being simply the best-known of these. All stages of stellar evolution from the main sequence to the ejection of a planetary nebula were considered, with emphasis on the changes that occur on the asymptotic giant branch. The spectroscopic properties of the photospheres and circumstellar envelopes of chemically-peculiar red giant stars, their origins via single-star ... Read more
The atmospheres of many stars have chemical compositions that are significantly different from that of the interstellar medium from which they are formed. This symposium considered all kinds of late-type stars showing altered compositions, the carbon stars being simply the best-known of these. All stages of stellar evolution from the main sequence to the ejection of a planetary nebula were considered, with emphasis on the changes that occur on the asymptotic giant branch. The spectroscopic properties of the photospheres and circumstellar envelopes of chemically-peculiar red giant stars, their origins via single-star ... Read more
Product Details
Format
Hardback
Publication date
2000
Publisher
Kluwer Academic Publishers United States
Number of pages
654
Condition
New
Series
International Astronomical Union Symposia (Closed)
Number of Pages
616
Place of Publication
Dordrecht, Netherlands
ISBN
9780792363460
SKU
V9780792363460
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
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