| B[e] Stars 1998 Edition Contributor(s): Hubert, Anne Marie (Editor), Jaschek, Carlos (Editor) |
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ISBN: 0792352084 ISBN-13: 9780792352082 Publisher: Springer OUR PRICE: $161.49 Product Type: Hardcover - Other Formats Published: September 1998 Annotation: These proceedings provide a broad overview of the research carried out to date on B-type stars with forbidden emission lines and dusty envelopes. These objects may represent an important transition stage in the evolution of many early-type stars, but they have been little studied until now. The book brings together the information available on the distribution, absolute magnitude, spectra in all wavelength ranges, photometric properties and variability of these objects. Also discussed are the different theoretical models proposed for explaining the amazing variety of phenomena observed. |
| Additional Information |
| BISAC Categories: - Science | Astronomy - Science | Physics - Astrophysics - Science | Physics - General |
| Dewey: 523.87 |
| LCCN: 98035406 |
| Series: Astrophysics and Space Science Library (Hardcover) |
| Physical Information: 0.75" H x 6.14" W x 9.21" (1.34 lbs) 289 pages |
| Descriptions, Reviews, Etc. |
| Publisher Description: The idea of having a meeting came to the Editors when working on several aspects of galactic Be and B e] stars. They found that a general summary of the properties of B e] stars was missing, so that the organiza- tion of a first meeting on these objects appeared as very useful. B e] stars have hydrogen line emission and forbidden Fe 11] and 0 I] emission lines in their spectra; they are also characterized by a strong IR excess due to circumstellar dust. Having a large amount of extinction in the UV and the visual they have been less frequently observed than other emission line objects. Although about one hundred galactic objects have been classified as B e], only fif- teen or so have been studied in some detail. Besides this, the evolutionary status of these objects is rat her controversial, are they pre-main sequence or stars on the way to become nUclei of planetary nebulae? Other difficult problems appear when considering the relations of these stars with other similar groups, like Herbig AeBe stars, Be, luminous blue variables and the superluminous B e] stars observed in the Magellanic Clouds. The conference seems timely since large surveys like DENIS and 2Mass, plus new space and new instruments for the micron, millimeter and cen- timeter wavelength region will result in the discovery of more stars of this group. |
