Atmósferas Estelares

The First Radio Spectrum of a Rapidly Rotating A-type Star

Presentamos el primer espectro en radio de una estrella de tipo espectral A.

White, Jacob Aaron, Francisco Tapia Vázquez, Hughes, A. G, Moór, A, Matthews, B, Wilner, D, Aufdenberg, J, Fehér, O, Hughes, A. M, De la Luz, V, McNaughton, A

The First Radio Spectrum of a Rapidly Rotating A-type Star

The MESAS Project: ALMA Observations of the F-type Stars γ Lep, γ Vir A, and γ Vir B

We present Atacama Large Millimeter/submillimeter Array observations of the three nearby, main-sequence, debris-poor, F-type stars γ Lep, γ Vir A, and γ Vir B at 0.87 and 1.29 mm.

White, Jacob Aaron, Francisco Tapia Vázquez, Hughes, A. G, Moór, A, Matthews, B, Wilner, D, Aufdenberg, J, Hughes, A. M, De la Luz, V, Boley, A. C

The MESAS Project: ALMA Observations of the F-type Stars γ Lep, γ Vir A, and γ Vir B

Nonlinear Convergence of Solar-like Stars Chromospheres Using Millimeter, Submillimeter, and Infrared Observations

In this work, we present a new methodology to fit the observed and synthetic spectrum of main-sequence stars through semiempirical models.

Francisco Tapia Vázquez, De la Luz, V

Nonlinear Convergence of Solar-like Stars Chromospheres Using Millimeter, Submillimeter, and Infrared Observations

ALMA's view of the nearest neighbors to the Sun. The submm/mm SEDs of the α Centauri binary and a new source

The precise mechanisms that provide the nonradiative energy for heating the chromosphere and corona of the Sun and other stars are at the focus of intense contemporary research.

Liseau, R, De la Luz, V, O'Gorman, E, Bertone, E, Chavez, M, Francisco Tapia Vázquez

ALMA's view of the nearest neighbors to the Sun. The submm/mm SEDs of the α Centauri binary and a new source

Measuring the Emission of Stellar Atmospheres at Submillimeter/millimeter wavelengths.

MESAS