Pulsations of the R Coronae Borealis stars
Cox, J. P. ; Wheeler, J. C. ; Hansen, C. J. ; King, D. S. ; Cox, A. N. ; Hodson, S. W.
Springer
Published 1980
Springer
Published 1980
ISSN: |
1572-9672
|
---|---|
Source: |
Springer Online Journal Archives 1860-2000
|
Topics: |
Physics
|
Notes: |
Abstract The radial pulsations of very luminous, low-mass models (L/M ∼ 104, solar units), which are possible representatives of the R CrB stars, have been examined. These pulsations are extremely nonadiabatic. We find that there are in some cases at least one extra (“strange”) mode which makes interpretation difficult. The blue instability edges are also peculiar, in that there is an abrupt excursion of the blue edge to the blue for L/M sufficiently large. The range of periods of the model encompasses observed periods of the Cepheid-like pulsations of actual R CrB stars.
|
Type of Medium: |
Electronic Resource
|
URL: |
_version_ | 1798296494790410240 |
---|---|
autor | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. |
autorsonst | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. |
book_url | http://dx.doi.org/10.1007/BF00168346 |
datenlieferant | nat_lic_papers |
hauptsatz | hsatz_simple |
identnr | NLM195925823 |
issn | 1572-9672 |
journal_name | Space science reviews |
materialart | 1 |
notes | Abstract The radial pulsations of very luminous, low-mass models (L/M ∼ 104, solar units), which are possible representatives of the R CrB stars, have been examined. These pulsations are extremely nonadiabatic. We find that there are in some cases at least one extra (“strange”) mode which makes interpretation difficult. The blue instability edges are also peculiar, in that there is an abrupt excursion of the blue edge to the blue for L/M sufficiently large. The range of periods of the model encompasses observed periods of the Cepheid-like pulsations of actual R CrB stars. |
package_name | Springer |
publikationsjahr_anzeige | 1980 |
publikationsjahr_facette | 1980 |
publikationsjahr_intervall | 8019:1980-1984 |
publikationsjahr_sort | 1980 |
publisher | Springer |
reference | 27 (1980), S. 529-535 |
search_space | articles |
shingle_author_1 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. |
shingle_author_2 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. |
shingle_author_3 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. |
shingle_author_4 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. |
shingle_catch_all_1 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. Pulsations of the R Coronae Borealis stars Abstract The radial pulsations of very luminous, low-mass models (L/M ∼ 104, solar units), which are possible representatives of the R CrB stars, have been examined. These pulsations are extremely nonadiabatic. We find that there are in some cases at least one extra (“strange”) mode which makes interpretation difficult. The blue instability edges are also peculiar, in that there is an abrupt excursion of the blue edge to the blue for L/M sufficiently large. The range of periods of the model encompasses observed periods of the Cepheid-like pulsations of actual R CrB stars. 1572-9672 15729672 Springer |
shingle_catch_all_2 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. Pulsations of the R Coronae Borealis stars Abstract The radial pulsations of very luminous, low-mass models (L/M ∼ 104, solar units), which are possible representatives of the R CrB stars, have been examined. These pulsations are extremely nonadiabatic. We find that there are in some cases at least one extra (“strange”) mode which makes interpretation difficult. The blue instability edges are also peculiar, in that there is an abrupt excursion of the blue edge to the blue for L/M sufficiently large. The range of periods of the model encompasses observed periods of the Cepheid-like pulsations of actual R CrB stars. 1572-9672 15729672 Springer |
shingle_catch_all_3 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. Pulsations of the R Coronae Borealis stars Abstract The radial pulsations of very luminous, low-mass models (L/M ∼ 104, solar units), which are possible representatives of the R CrB stars, have been examined. These pulsations are extremely nonadiabatic. We find that there are in some cases at least one extra (“strange”) mode which makes interpretation difficult. The blue instability edges are also peculiar, in that there is an abrupt excursion of the blue edge to the blue for L/M sufficiently large. The range of periods of the model encompasses observed periods of the Cepheid-like pulsations of actual R CrB stars. 1572-9672 15729672 Springer |
shingle_catch_all_4 | Cox, J. P. Wheeler, J. C. Hansen, C. J. King, D. S. Cox, A. N. Hodson, S. W. Pulsations of the R Coronae Borealis stars Abstract The radial pulsations of very luminous, low-mass models (L/M ∼ 104, solar units), which are possible representatives of the R CrB stars, have been examined. These pulsations are extremely nonadiabatic. We find that there are in some cases at least one extra (“strange”) mode which makes interpretation difficult. The blue instability edges are also peculiar, in that there is an abrupt excursion of the blue edge to the blue for L/M sufficiently large. The range of periods of the model encompasses observed periods of the Cepheid-like pulsations of actual R CrB stars. 1572-9672 15729672 Springer |
shingle_title_1 | Pulsations of the R Coronae Borealis stars |
shingle_title_2 | Pulsations of the R Coronae Borealis stars |
shingle_title_3 | Pulsations of the R Coronae Borealis stars |
shingle_title_4 | Pulsations of the R Coronae Borealis stars |
sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
source_archive | Springer Online Journal Archives 1860-2000 |
timestamp | 2024-05-06T09:52:59.867Z |
titel | Pulsations of the R Coronae Borealis stars |
titel_suche | Pulsations of the R Coronae Borealis stars |
topic | U |
uid | nat_lic_papers_NLM195925823 |