Showing 2004 · astro-phShow all

31 papers · 2 filters

astro-ph2004★ 48 cited

Evidence for a hot dust-free inner disk around 51 Oph

W. -F. Thi, B. van Dalen, A. Bik +1

We report on the observation of CO bandhead emission around 51 Oph (dv=2). A high resolving power (R~10,000) spectrum was obtained with the infrared spectrometer ISAAC mounted on V…

astro-ph2004★ 10 cited

The influence of chemical composition on the properties of Cepheid stars I - Period-Luminosity relation vs iron abundance

M. Romaniello, F. Primas, M. Mottini +3

We have assessed the influence of the stellar iron content on the Cepheid Period-Luminosity (PL) relation by relating the V band residuals from the Freedman et al (2001) PL relatio…

astro-ph2004★ 5 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-ph2004★ 29 cited

Radiatively driven rotating pair-plasma jets from two component accretion flows

Indranil Chattopadhyay

Centrifugal pressure of matter spiralling onto black holes, have long been known to produce standing or oscillating shocks. The post-shock disc puffs up in the form of a torus, whi…

astro-ph2004★ 1 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-ph2004★ 35 cited

Orbital parameters, masses and distance to Beta Centauri determined with the Sydney University Stellar Interferometer and high resolution spectroscopy

J. Davis, A. Mendez, E. B. Seneta +7

The bright southern binary star beta Centauri (HR 5267) has been observed with the Sydney University Stellar Interferometer (SUSI) and spectroscopically with the ESO CAT and Swiss…

astro-ph2004★ 1 cited

How to reconcile the C and s-process abundances in the metal-poor star V453 Oph ?

Pieter Deroo, Stephane Goriely, Lionel Siess +2

In this poster we present a detailed chemical analysis of the RV Tauri star of low intrinsic metallicity, V453 Oph ([Fe/H]=-2.2), which shows a mild but clear s-process surface ove…

astro-ph2004★ 1 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★ 39 cited

GAUDI: a preparatory archive for the COROT mission

E. Solano, C. Catala, R. Garrido +34

The GAUDI database (Ground-based Asteroseismology Uniform Database Interface, http://sdc.laeff.esa.es/gaudi/) is a preparatory archive for the COROT (COnvection, ROtation and plane…

astro-ph2004★ 42 cited

The distance to the Pleiades: Main sequence fitting in the near infrared

S. M. Percival, M. Salaris, M. A. T. Groenewegen

Hipparcos parallax measurements of stars in the Pleiades notoriously result in a cluster distance of 118 pc; ~10% shorter than the `classical' results of MS-fitting. In an earlier…

astro-ph2004★ 252 cited

A purely geometric distance to the binary star Atlas, a member of the Pleiades

N. Zwahlen, P. North, Y. Debernardi +4

We present radial velocity and new interferometric measurements of the double star Atlas, which permit, with the addition of published interferometric data, to precisely derive the…

astro-ph2004★ 68 cited

Chemical analysis of 24 dusty (pre-)main-sequence stars

Bram Acke, Christoffel Waelkens

We have analysed the chemical photospheric composition of 24 Herbig Ae/Be and Vega-type stars in search for the lambda Bootis phenomenon. We present the results of the elemental ab…

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★ 12 cited

'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 Alfven waves (Zaqarashvili and Roberts 2002) is generalized to inhomogeneous media. We show that the fast mag…

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…

astro-ph2004★ 34 cited

Improved Baade-Wesselink surface-brightness relations

Martin Groenewegen

Recent, and older accurate, data on (limb-darkened) angular diameters is compiled for 221 stars, as well as BVRIJK[12][25] magnitudes for those objects, when available. Nine stars…

astro-ph2004★ 54 cited

MARCS-Model Stellar Atmospheres, and Their Application to the Photometric Calibration of the Spitzer-IRS

L. Decin, P. W. Morris, P. N. Appleton +3

We describe state-of-the-art MARCS-code model atmospheres generated for a group of A dwarf, G dwarf, and late-G to mid-K giant standard stars, selected to photometrically calibrate…

astro-ph2004★ 257 cited

ISO spectroscopy of disks around Herbig Ae/Be stars

Bram Acke, Mario E. van den Ancker

We have investigated the infrared spectra of all 46 Herbig Ae/Be stars for which spectroscopic data is available in the ISO data archive. Our quantitative analysis of these spectra…

astro-ph2004★ 283 cited

The profiles of the 3 to 12 m PAH features

B. van Diedenhoven, E. Peeters, C. Van Kerckhoven +4

We present spectra of the 3.3 m and 11.2 m PAH features of a large number of (extra-) galactic sources, obtained with ISO-SWS. Clear variations are present in the profiles of…

astro-ph2004★ 74 cited

Long Period Variables in the Magellanic Clouds: OGLE + 2MASS + DENIS

Martin Groenewegen

(abridged) The 68000 I-band light curves of variable stars detected by the OGLE survey in the Large and Small Magellanic Clouds (MCs) are fitted by Fourier series, and also correla…

astro-ph2004★ 97 cited

Correlation between grain growth and disk geometry in Herbig Ae/Be systems

B. Acke, M. E. van den Ancker, C. P. Dullemond +2

We have calculated the (sub-)mm spectral indices of 26 Herbig Ae/Be stars, for which we can determine the infrared spectral energy distribution (SED). We find a clear correlation b…

astro-ph2004★ 76 cited

Evolution of planetary nebulae II. Population effects on the bright cut-off of the PNLF

P. Marigo, L. Girardi, A. Weiss +2

We investigate the bright cut-off of the [OIII]l5007 planetary nebula luminosity function (PNLF), that has been suggested as a powerful extragalactic distance indicator. Theoretica…

astro-ph2004★ 43 cited

The metallicity dependence of the Cepheid PL-relation

M. A. T. Groenewegen, M. Romaniello, F. Primas +1

A sample of 37 Galactic, 10 LMC and 6 SMC cepheids is compiled for which individual metallicity estimates exist and BVIK photometry in almost all cases. The Galactic cepheids all h…