Related content

Determining parameters of cool giant stars by modeling spectrophotometric and interferometric observations using the SAtlas program

By  

Astronomy & Astrophysics, Vol. 490, Iss. 2, 2008-11 ,pp. : 807-810 (4)

Edp Sciences

Access to resources Recommend Favorite

A new method to compute limb-darkening coefficients for stellar atmosphere models with spherical symmetry: the space missions TESS, Kepler, CoRoT, and MOST⋆⋆⋆

By Claret Antonio  

Astronomy & Astrophysics, Vol. 618, Iss. issue, 2018-10 ,pp. : A20-A20 (NaN)

Edp Sciences

Access to resources Recommend Favorite

Proof that static stellar models are spherical

By Masood-ul-Alam A.  

General Relativity and Gravitation, Vol. 39, Iss. 1, 2007-01 ,pp. : 55-85 (31)

Springer Publishing Company

Access to resources Recommend Favorite

Stability of rotating spherical stellar systems

By  

Astronomy & Astrophysics, Vol. 395, Iss. 1, 2002-11 ,pp. : 25-30 (6)

Edp Sciences

Access to resources Recommend Favorite

Limb darkening in spherical stellar atmospheres

By Neilson H. R.   Lester J. B.  

Astronomy & Astrophysics, Vol. 530, Iss. issue, 2011-05 ,pp. : A65-A65 (NaN)

Edp Sciences

Access to resources Recommend Favorite