Near Infrared Lines as Diagnostics of Accretion in T Tauri Stars

ISSN： 0004-640X

Source： Astrophysics and Space Science, Vol.261, Iss.1-4, 1998-01, pp. : 147-150

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

Abstract

Related content

The frequency of large variations in the near-infrared fluxes of T Tauri stars

By Scholz Alexander

Monthly Notices of the Royal Astronomical Society, Vol. 420, Iss. 2, 2012-02 ,pp. : 1495-1502

Oxford University Press

Access to resources Recommend Favorite

On the nature of the spectrum veiling for classical T Tauri stars in the near infrared

By Dodin A. Lamzin S.

Astronomy Letters, Vol. 39, Iss. 6, 2013-06 ,pp. : 389-392

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Time Dependent Magnetospheric Accretion in T Tauri Stars

By Bouvier J.

Astrophysics and Space Science, Vol. 292, Iss. 1-4, 2004-08 ,pp. : 659-664

Springer Publishing Company

Access to resources Recommend Favorite

Calculation of profiles of CIV, NV, OVI, and SiIV resonance lines formed in accretion shocks in T Tauri stars: A plane layer

By Lamzin S.

Astronomy Reports, Vol. 47, Iss. 6, 2003-06 ,pp. : 498-510

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

X Rays and UV Emission Lines in T Tauri Stars

By Huélamo N. de Castro A.I.G. Franqueira M.

Astrophysics and Space Science, Vol. 261, Iss. 1-4, 1998-01 ,pp. : 127-128

Springer Publishing Company

Access to resources Recommend Favorite