The Carbon Star Phenomenon

Proceedings of the 177th Symposium of the International Astronomical Union, held in Antalya, Turkey, May 27-31, 1996

The Carbon Star Phenomenon

Author: International Astronomical Union. Symposium

Publisher: Springer Science & Business Media

ISBN: 9780792363460

Page: 613

View: 269

Proceedings of the 177th Symposium of the International Astronomical Union, held in Antalya, Turkey, May 27-31, 1996

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 ...

Stars with the B e  Phenomenon

Author: Michaela Kraus

Publisher: Astronomical Society of the pacific

ISBN:

Page: 385

View: 104

Dust and Molecules in Evolved Stars

References Asplund, M., 1997, In Ed., R.F. Wing, The Carbon Star Phenomenon,
IAU Symposium 177, Kluwer, in press Böhm-Vitense, E., 1990, Stellar
Astrophysics, Vol.2, Cambridge. Birdsall, C.K., Langdon, A.B., 1985, Plasma
Physics via ...

Dust and Molecules in Evolved Stars

Author: I. Cherchneff

Publisher: Springer Science & Business Media

ISBN: 9401713073

Page: 396

View: 674

Dust and molecules are found in a large variety of astrophysical environments, in particular in the circumstellar material ejected by evolved stars. This book brings together the leading astronomers and astrophysicists in the field of molecular astrophysics and stellar physics to discuss the important issues of dust and molecular formation, the role of solids in circumstellar environments, molecules as probes of circumstellar parameters, the stellar contribution to the enrichment of the Galaxy, and the latest observational data in various wavelength domains, in partiular in the infrared with results from the Infrared Space Observatory. The astrophysical senarios include late-type stars, novae, Wolf-Rayet stars, Luminous Blue Variables and supernovae. Audience: Researchers and graduate students in the fields of stellar physics, stellar evolution and astrochemistry.

Carbon Stars

The latter phenomenon is currently detected only in M - class Miras . Gorbatskií (
1961 ) developed a theory for the propagation of shock waves in stellar
atmospheres which provides a good explanation for the origin of the emission
spectra ...

Carbon Stars

Author: Zenta Alksne

Publisher:

ISBN:

Page: 182

View: 134

Asymptotic Giant Branch Stars

Sp . Sci 255 , 267 Blöcker T . , 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 . R . Wing , Kluwer , Dordrecht , in press
Boothroyd A . D ...

Asymptotic Giant Branch Stars

Author: International Astronomical Union. Symposium

Publisher: Astronomical Society of the pacific

ISBN:

Page: 632

View: 814

The nonprofit Astronomical Society of the Pacific (ASP) publishes the Conference Series Proceedings as part of its century-old mission to provide resources for astronomers and advance the science of astronomy. Since 1988, the ASP has published the proceedings of astronomical workshops, meetings, colloquia, and symposia to meet the community's demand for affordable, high-quality volumes on current topics in the rapidly expanding fields of astronomy and astrophysics. Since 1998, the Society has also served as publisher for the International Astronomical Union (IAU), adding their Symposia, Highlights, and Transactions to our growing list of publications.For most rapid delivery of each volume, we encourage libraries and astronomy departments to place a Standing Order for the ASP Conference Series and/or the IAU Publications. Standing Orders are shipped directly from the printer and customers receive volumes at the same discounted rates as ASP members (approximately 25-35 ASP volumes each year and/or 5 IAU Symposia). Please refer to the order form to take advantage of this time-saving offer.We encourage all professionals who are sponsoring conferences, workshops, or colloquia to inquire about publishing these proceedings with the ASP. We provide quality volumes at less than half the price of comparable titles from other major publishers, ensuring that the publication will be available to a wider audience of budget-conscious scientists.Held in Montpellier, France, 27 August - 1 September 1998.

McGraw Hill Encyclopedia of Science Technology

Carbon star Any of a class of stars with an apparently high abundance ratio of
carbon to hydrogen. In normal stars, oxygen is ... varies from star to star. In a
related phenomenon found in global clusters, variations in the C/N/O ratios are
found.

McGraw Hill Encyclopedia of Science   Technology

Author:

Publisher:

ISBN:

Page:

View: 480

The Harlow Shapley Symposium on Globular Cluster Systems in Galaxies

Their integrated spectral types are GO , G4 and late F . RICHER : Your comment
about the M 33 clusters being a good place to look for the onset of the carbon star
phenomenon , is this based on the fact that the age distribution is more ...

The Harlow Shapley Symposium on Globular Cluster Systems in Galaxies

Author: Jonathan E. Grindlay

Publisher: Springer

ISBN: 9789027726643

Page: 780

View: 996

In the centennial year, 1985-86, of Harlow Shapley's birth, the study of globular clusters was no less important to the development of astronomy than in 1915, when Shapley first noted their concentration on the sky. By 1917 Shapley had used the properties of the system of globular clusters to complete the Copernican revolution and locate the solar system, and its Earth-bound observers, far from the center of the Galaxy and the globular cluster distribution. Seven decades later, in the year of these proceedings, globular cluster research and the study of the system of globular clusters in our own and distant galaxies is undergoing a renaissance of activity. The introduction of new observational tools, particularly CCD imagers and digital spectrographs, as well as powerful theoretical methods have transformed the study of globular clusters into one of the main line areas of modern astrophysics. Thus it seemed particularly appropriate to one of us, when considering how the Harvard College Observatory might mark the Shapley centennial, to propose and plan for an IAU Symposium on Globular Cluster Systems in Galaxies. Planning for the Shapley Symposium, as it came to be called, was even more drawn out than the preparation of this volume. The Symposium was originally proposed to the IAU Secretariat in time for it to be held in August, 1985, so that it might occur in the centennial (calendar) year.

Diffuse Infrared Radiation and the IRTS

... Springer , 79 Tsuji , T . 1997 , in The Carbon Star Phenomenon , R . F . Wing ,
Kluwer , in press Tsuji , T . , Ohnaka , K . , Hinkle , K . H . , & Ridgway , S . T . 1994
, A & A , 289 , 469 Tsuji , T . , Ohnaka , K . , & Aoki , W . 1996a , A & A , 305 , L1 ...

Diffuse Infrared Radiation and the IRTS

Author: Haruyuki Okuda

Publisher: Astronomical Society of the pacific

ISBN:

Page: 497

View: 274

Vistas in Astronomy

THE VELOCITY BODY OF CARBON STARS During the investigation of peculiar
motions of carbon stars ( stars of spectral class R and N , designated ... This
phenomenon is connected with the problem of stars escaping ( parabolic velocity
) .

Vistas in Astronomy

Author:

Publisher:

ISBN:

Page:

View: 778

Information Bulletin on Variable Stars

1993 ) , a condensation of carbon dust which is not a rare phenomenon in the
atmosphere of hydrogen deficient carbon stars ( Warner 1967 ) . This scenario is
consistent with the increasing of the infrared flux and the lack of the emission ...

Information Bulletin on Variable Stars

Author:

Publisher:

ISBN:

Page:

View: 567

Annual Report

In : The Carbon Star Phenomenon . ( Ed . ) R.F. Wing . ... In : Birth and Evolution
of Binary Stars . ( Eds ) B. Reipurth ... Rudnick , G. , H.-W. Rix and R.C.J.
Kennicutt : Lopsided Galaxies , Weak Interactions and Boosting the Star
Formation Rate .

Annual Report

Author: Max-Planck-Institut für Astronomie

Publisher:

ISBN:

Page:

View: 453

Les processus nucl aires dans les astres

much weaker in these stars than in other carbon stars these objects appear to be
cases of a carbon abundance ... thinking that the apparent high abundance of
carbon in the carbon stars is a real , rather than a spectroscopic , phenomenon .

Les processus nucl  aires dans les astres

Author:

Publisher:

ISBN:

Page: 546

View: 739