Profil

Ouazzani Rhita-Maria

See author's contact details
Main Referenced Co-authors
Dupret, Marc-Antoine  (4)
Reese, Daniel  (2)
Roxburgh, I. W. (2)
Goupil, M. J. (1)
Goupil, M.-J. (1)
Main Referenced Keywords
asteroseismology (2); Astrophysics - Solar and Stellar Astrophysics (2); methods: numerical (1); oscillations (1); rotation (1);
Main Referenced Disciplines
Space science, astronomy & astrophysics (5)

Publications (total 5)

The most downloaded
34 downloads
Ouazzani, R.-M., & Goupil, M.-J. (June 2012). Rotational splittings for slow to moderate rotators. Latitudinal dependence or higher order effects in Ω? Astronomy and Astrophysics, 542 (A99). doi:10.1051/0004-6361/201117151 https://hdl.handle.net/2268/142500

The most cited

47 citations (Scopus®)

Ouazzani, R.-M., Dupret, M.-A., & Reese, D. (01 November 2012). Pulsations of rapidly rotating stars. I. The ACOR numerical code. Astronomy and Astrophysics, 547, 75. doi:10.1051/0004-6361/201219548 https://hdl.handle.net/2268/140167

Ouazzani, R.-M., Dupret, M.-A., & Reese, D. (01 November 2012). Pulsations of rapidly rotating stars. I. The ACOR numerical code. Astronomy and Astrophysics, 547, 75. doi:10.1051/0004-6361/201219548
Peer Reviewed verified by ORBi

Ouazzani, R.-M., Dupret, M.-A., Roxburgh, I. W., & Goupil, M.-J. (2012). Pulsations of an Evolved Self-consistently Distorted Star. In ASP Conference Proceeding, Vol. 462, 402 (pp. 402).

Ouazzani, R.-M., & Goupil, M.-J. (June 2012). Rotational splittings for slow to moderate rotators. Latitudinal dependence or higher order effects in Ω? Astronomy and Astrophysics, 542 (A99). doi:10.1051/0004-6361/201117151
Peer Reviewed verified by ORBi

Ouazzani, R.-M., Roxburgh, I. W., & Dupret, M.-A. (01 January 2012). Pulsations of rapidly rotating evolved stars. proceedings of the 20th Stellar Pulsation Conference Series, Granada sept 2011, 1301, 2496.

Ouazzani, R.-M., Dupret, M.-A., Goupil, M. J., & Reese, D. (01 January 2010). 2D non-perturbative modeling of oscillations in rapidly rotating stars. Astronomical Notes, 331, 45.

Contact ORBi