Proceedings of the Conference on Red Giant Stars
This upper limit would be the main sequence life - time of an FSV star ( 1 . 4 solar
masses : Allen 1963 ) , or approximately 1 . 6x10° years ( Iben 1967 ) . If the 2 S
carbon star phenomenon is representative of a stage of stellar evolution beyond
...
Author: Hollis Ralph Johnson
Publisher:
ISBN:
Page: 535
View: 826
Dissertation Abstracts International
SAAO Newsletter
Properties of Galactic Carbon Stars
It turned out that in cold stars with T , < 4000° K and an extended convective zone
, an important part is played by dipole and especially monopole sound radiation
... In the spectra of studied carbon stars , no such phenomena were observed .
Author: Zenta Alksne
Publisher:
ISBN:
Page: 163
View: 907
South African Astronomical Observatory Report for the Year Ending
Why Galaxies Care about AGB Stars
Stars with the B e Phenomenon
355 , 2006 Michaela Kraus and Anatoly S . Miroshnichenko The Unusual
Emission Line Star V 439 Cyg in Berkeley 87 V . F . Polcaro Istituto di Astrofisica
Spaziale e Fisica Cosmica , INAF , Roma , Italy L . Norci Dublin City University ,
Dublin ...
Author: Michaela Kraus
Publisher: Astronomical Society of the pacific
ISBN:
Page: 385
View: 234
STAR
Bulletin of the Astronomical Society of India
Do inhabitants of the planets responsible for such secondary dust pay special
attention to the star patterns through which their host ... 2001 , 2003 , 2004 ) , but
in general this is a phenomenon that difinitely exists , but the composition is
probably the cause of the ... Oxygen - bearing molecules in the spectra of carbon
stars .
Author:
Publisher:
ISBN:
Page:
View: 412
Cool Stars Stellar Systems and the Sun
Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems
and the Sun Eric Stempels. E DY Per September 2004 NaI 012 1 . ... 177 , The
Carbon Star Phenomenon , edited by R . F . Wing , Kluwer , Dordrecht , 2000 , pp
.
Author: Eric Stempels
Publisher: American Institute of Physics
ISBN:
Page: 992
View: 441
1997 Pacific Rim Conference on Stellar Astrophysics
The Galaxy and the Local Group
Royal Greenwich Observatory Bulletins
The particular mechanism we have in mind for producing the carbon star
phenomenon is that suggested by Iben ( 1975 ) . ( d ) Population II Stars with
Rotating Cores We have recently incorporated in equations ( 5 ) and ( 7 ) the
effects of the ...
Author: Royal Greenwich Observatory
Publisher:
ISBN:
Page:
View: 917
The Galaxy and the Local Group
The particular mechanism we have in mind for producing the carbon star
phenomenon is that suggested by Iben ( 1975 ) . ( d ) Population II Stars with
Rotating Cores We have recently incorporated in equations ( 5 ) and ( 7 ) the
effects of the ...
Author: R. J. Dickens
Publisher:
ISBN:
Page: 293
View: 472
Nuclear Science Abstracts
Hydrogen deficient Stars
explain the observational fact that nonradial pulsations are reported for the
hottest EHe - B stars ( V2205 Oph , V2076 Oph ) , while no nonradial pulsations
are found in R CrB stars . 4 . Conclusion ... 177 , The Carbon Star Phenomenon ,
ed .
Author: Klaus Werner
Publisher: Astronomical Society of the pacific
ISBN:
Page: 384
View: 589
World Meetings Outside U S A and Canada
Asymptotic Giant Branch Stars
the structure and evolution of AGB stars remains to be investigated in more detail
. ... Schönberner , D . , 1991 , A & A 244 , L43 Blöcker T . , Herwig F . ,
Schönberner D . , El Eid M . , 1998 , The Carbon Star Phenomenon , IAU Symp .
177 , ed .
Author: International Astronomical Union. Symposium
Publisher: Astronomical Society of the pacific
ISBN:
Page: 632
View: 738