Equidistant frequency triplets in pulsating stars: the combination mode hypothesis

Publisher： Edp Sciences

E-ISSN： 1432-0746|460|1|167-172

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.460, Iss.1, 2006-12, pp. : 167-172

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Breaking the core-envelope symmetry in p-mode pulsating stars

By  

Astronomy & Astrophysics, Vol. 422, Iss. 1, 2004-07 ,pp. : 271-273

Edp Sciences

Access to resources Recommend Favorite

Non-radially pulsating Be stars

By  

Astronomy & Astrophysics, Vol. 411, Iss. 2, 2003-11 ,pp. : 229-247

Edp Sciences

Access to resources Recommend Favorite

Pulsating stars in NGC 6231

By Meingast Stefan   Handler Gerald   Shobbrook Robert R.  

Astronomy & Astrophysics, Vol. 559, Iss. issue, 2013-11 ,pp. : A108-A108

Edp Sciences

Access to resources Recommend Favorite

Fourier decomposition and frequency analysis of the pulsating stars with $P < $ 1 d in the OGLE database

By  

Astronomy & Astrophysics, Vol. 398, Iss. 1, 2003-01 ,pp. : 213-222

Edp Sciences

Access to resources Recommend Favorite

Fourier decomposition and frequency analysis of the pulsating stars with$\vec{P< }$ 1 d in the OGLE database

By  

Astronomy & Astrophysics, Vol. 371, Iss. 3, 2001-06 ,pp. : 986-996

Edp Sciences

Access to resources Recommend Favorite