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astro-ph20045 cited

The evolutionary status of the bright high-latitude supergiant HD190390

Maarten Reyniers, Jan Cuypers

Despite its mean apparent magnitude of m(v)=6.39, the evolutionary status of HD190390 (HR7671), a luminous F-type supergiant at high galactic latitude, is still not very clear, but…

astro-ph20041 cited

The Metallicity dependence of the Cepheid Period-Luminosity relation: methodology and results

Marta Mottini, Martino Romaniello, Francesca Primas +3

We present the results of an observational campaign undertaken to assess the influence of the iron content on the Cepheid Period-Luminosity relation. Our data indicate that this de…

astro-ph20041 cited

Is the solar corona nonmodally self-heated?

B. M. Shergelashvili, A. D. Rogava, S. Poedts

Recently it was pointed out that nonmodally (transiently and/or adiabatically) pre-amplified waves in shear flows, undergoing subsequent viscous damping, can ultimately heat the am…

astro-ph2004

The mechanism of Swing Absorption of fast magnetosonic waves in inhomogeneous media

B. M. Shergelashvili, T. V. Zaqarashvili, S. Poedts +1

The recently suggested swing interaction between fast magnetosonic and Alfvén waves (2002) is generalized to inhomogeneous media. We show that the fast magnetosonic waves propagati…

astro-ph2004

[O I] 6300 A Emission from Disks Around Herbig Ae/Be Stars

M. E. van den Ancker, B. Acke, C. P. Dullemond

We present high spectral-resolution optical spectra of 49 Herbig Ae/Be stars in a search for the [O I] 6300.2 A line. The vast majority of the stars in our sample show narrow (FWHM…

astro-ph2004

AGB stars in the Local Group, and beyond

Martin Groenewegen

I summarize the current status of surveys for late-type M, and Carbon stars in the Local Group based on three different approaches that make use of the characteristics of these sta…