On the pulsation modes and masses of RGB OSARGs
OSARG (OGLE Small Amplitude Red Giants) variables are RGB or AGB stars that show multi-periodic light variations with periods of about 10-100 days. Comparing linear nonadiabatic pulsation periods and period ratios with observed ones, we determined pulsation modes and masses of the RGB OSARG variable...
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EDP Sciences
2013-03-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20134303013 |
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doaj-521ce144f0074b138b7f7e85bac7013a2021-08-02T06:56:47ZengEDP SciencesEPJ Web of Conferences2100-014X2013-03-01430301310.1051/epjconf/20134303013On the pulsation modes and masses of RGB OSARGsSaio H.Takayama M.Ita Y.OSARG (OGLE Small Amplitude Red Giants) variables are RGB or AGB stars that show multi-periodic light variations with periods of about 10-100 days. Comparing linear nonadiabatic pulsation periods and period ratios with observed ones, we determined pulsation modes and masses of the RGB OSARG variables in the LMC. We found that pulsations of OSARGs involve radial 1st to 3rd overtones, p4 of l = 1, and p2 of l = 2 modes. The range of mass isfound to be 0.9-1.4M⊙ for RGB OSARGs and their mass-luminosity relation is logL/L⊙ = 0.79 M/M⊙ + 2.2. http://dx.doi.org/10.1051/epjconf/20134303013 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Saio H. Takayama M. Ita Y. |
| spellingShingle |
Saio H. Takayama M. Ita Y. On the pulsation modes and masses of RGB OSARGs EPJ Web of Conferences |
| author_facet |
Saio H. Takayama M. Ita Y. |
| author_sort |
Saio H. |
| title |
On the pulsation modes and masses of RGB OSARGs |
| title_short |
On the pulsation modes and masses of RGB OSARGs |
| title_full |
On the pulsation modes and masses of RGB OSARGs |
| title_fullStr |
On the pulsation modes and masses of RGB OSARGs |
| title_full_unstemmed |
On the pulsation modes and masses of RGB OSARGs |
| title_sort |
on the pulsation modes and masses of rgb osargs |
| publisher |
EDP Sciences |
| series |
EPJ Web of Conferences |
| issn |
2100-014X |
| publishDate |
2013-03-01 |
| description |
OSARG (OGLE Small Amplitude Red Giants) variables are RGB or AGB stars that show multi-periodic light variations with periods of about 10-100 days. Comparing linear nonadiabatic pulsation periods and period ratios with observed ones, we determined pulsation modes and masses of the RGB OSARG variables in the LMC. We found that pulsations of OSARGs involve radial 1st to 3rd overtones, p4 of l = 1, and p2 of l = 2 modes. The range of mass isfound to be 0.9-1.4M⊙ for RGB OSARGs and their mass-luminosity relation is logL/L⊙ = 0.79 M/M⊙ + 2.2. |
| url |
http://dx.doi.org/10.1051/epjconf/20134303013 |
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