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Przemysław Walczak Jadwiga Daszyńska-Daszkiewicz Uniwersytet Wrocławski Instytut Astronomiczny, Poland Wrocław, 21.08.2013. Testing microphysics data. β Cephei stars. θ Ophiuchi ν Eridani γ Pegasi 12 Lacertae. Asteroseismic tools. ν pulsational frequency f -parameter.
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Przemysław Walczak Jadwiga Daszyńska-Daszkiewicz Uniwersytet Wrocławski Instytut Astronomiczny, Poland Wrocław, 21.08.2013 Testing microphysics data
βCepheistars • θOphiuchi • νEridani • γPegasi • 12 Lacertae
Asteroseismictools νpulsationalfrequency f-parameter
fresultsfromlinear, nonadiabaticcomputations of stellaroscillations the nonadiabatic, complex parameter f a ratio of thebolometricfluxperturbation to theradialdisplacementatthephotospherelevel
frequency, stellar parameters, M, Teff shape of eigenfunctions chemical composition, (X, Z, mixture) opacity subphotosphericconvection rotation, if Values of f depend on:
Method of determination of f Daszyńska-Daszkiewicz, J., Dziembowski, W. A., Pamyatnykh, A. A, 2003, A&A 407, 999 (for δScutistars) Daszyńska-Daszkiewicz, J., Dziembowski, W. A., Pamyatnykh, A. A, 2005, A&A 441, 641 (for βCepheistars)
Method of determination of f Daszyńska-Daszkiewicz, J., Dziembowski, W. A., Pamyatnykh, A. A, 2003, A&A 407, 999 (for δScutistars) Daszyńska-Daszkiewicz, J., Dziembowski, W. A., Pamyatnykh, A. A, 2005, A&A 441, 641 (for βCepheistars)
OP: H, He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Cr, Mn, Fe, Ni OPACITY TABLES (Seaton, 2005, MNRAS, 362, L1)
OP: H, He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Cr, Mn, Fe, Ni OPAL:H, He, C, N, O, Ne, Na, Mg, Al, Si, P, S, Cl, Ar, K, Ca, Ti, Cr, Mn, Fe, Ni OPACITY TABLES (Iglesias & Rogers 1996, ApJ 464, 943)
OP: H, He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Cr, Mn, Fe, Ni OPAL:H, He, C, N, O, Ne, Na, Mg, Al, Si, P, S, Cl, Ar, K, Ca, Ti, Cr, Mn, Fe, Ni LA: H, He, Li,Be,B, C, N, O, F, Ne, Na, Mg, Al, Si, P, S, Cl, Ar, K, Ca, Sc, Ti, V, Cr, Mn, Fe,Co, Ni, Cu, Zn OPACITY TABLES (Magee et al. 1995, in ASP Conf. Ser. 78, 51)
HD157056 V = 3.25 mag B2IV θOphiuchi Briquet, M., Lefever, K., Uytterhoeven, K., Aerts, C. , 2005, MNRAS, 362, 619 Handler, G., Shobbrook, R. R., Mokgwetsi, T., 2005, MNRAS 362, 612
HD157056 V = 3.25 mag B2IV θOphiuchi Briquet, M., Lefever, K., Uytterhoeven, K., Aerts, C. , 2005, MNRAS, 362, 619 Handler, G., Shobbrook, R. R., Mokgwetsi, T., 2005, MNRAS 362, 612
ν3= 7.4677 c/d l=0, ν6= 7.8742 c/d l=1 θOphiuchi
ν3= 7.4677 c/d l=0, ν6= 7.8742 c/d l=1 θOphiuchi OP (Seaton 2005)
ν3= 7.4677 c/d l=0, ν6= 7.8742 c/d l=1 θOphiuchi
ν3= 7.4677 c/d l=0, ν6= 7.8742 c/d l=1 θOphiuchi OP (Seaton 2005)
HD 886 V=2.83 mag B2IV γPegasi Handler, G.: 2009, MNRAS 398, 1339; Handler, G., Matthews, J.M., Eaton, J.A. et al.: 2009, ApJ 698, 56
HD 886 V=2.83 mag B2IV γPegasi Handler, G.: 2009, MNRAS 398, 1339; Handler, G., Matthews, J.M., Eaton, J.A. et al.: 2009, ApJ 698, 56
HD 214993 V = 5.228 mag B2III 12 Lacertae Desmet M., Briquet M., Thoul A., et al., 2009, MNRAS,396, 1460 Handler, G., Jerzykiewicz, M., Rodriguez, E., at al., 2006, MNRAS, 365, 327
HD 214993 V = 5.228 mag B2III 12 Lacertae Desmet M., Briquet M., Thoul A., et al., 2009, MNRAS,396, 1460 Handler, G., Jerzykiewicz, M., Rodriguez, E., at al., 2006, MNRAS, 365, 327
ν4=5.334357 c/d l=0, ν2=5.066346 c/d l=1 12 Lacertae
ν4=5.334357 c/d l=0, ν2=5.066346 c/d l=1 12 Lacertae
ν4=5.334357 c/d l=0, ν2=5.066346 c/d l=1 12 Lacertae
ν4=5.334357 c/d l=0, ν2=5.066346 c/d l=1 12 Lacertae Morel T., Butler K., Aerts C., Neiner C., Briquet M., 2006, A&A, 457, 651
12 Lacertae ν4=5.334357 c/d l=0, ν2=5.066346 c/d l=1 50%
12 Lacertae ν4=5.334357 c/d l=0, ν2=5.066346 c/d l=1 50%
HD 29248 • V = 3.92 mag • B2III ν ERIDANI Aerts C., de Cat P., Handler G., et al., 2004, MNRAS, 347, 463 Jerzykiewicz M., Handler G., Shobbrook R. R., et al., 2005, MNRAS 360, 619
HD 29248 • V = 3.92 mag • B2III ν ERIDANI Aerts C., de Cat P., Handler G., et al., 2004, MNRAS, 347, 463 Jerzykiewicz M., Handler G., Shobbrook R. R., et al., 2005, MNRAS 360, 619
ν1 = 5.7632828 c/d l=0, ν4 = 5.6372470 c/d l=1, ν6 = 6.243847 c/d l=1 ν ERIDANI
ν1 = 5.7632828 c/d l=0, ν4 = 5.6372470 c/d l=1, ν6 = 6.243847 c/d l=1 ν ERIDANI
ν1 = 5.7632828 c/d l=0, ν4 = 5.6372470 c/d l=1, ν6 = 6.243847 c/d l=1 ν ERIDANI
ν1 = 5.7632828 c/d l=0 ν ERIDANI
νB=0.61440 c/d, l=2 ν ERIDANI
θ Oph: OPAL(LA) • γ Peg: no preferences • 12 Lac: OP • ν Eri: • High frequency modes: OPAL/LA • Low frequency mode: OP • LA – excitationproblems Summary
βCepheistars Mass: 8-17 Msun • Spectral type:O8-B6 • Light amplitudes: 0.01 - 0.3 magnitudes • Periods: 0.1 - 0.6 days (~2 – 15 hours)