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Constraints on the use of Be I lines for deriving beryllium abundances in late-type dwarf stars. |
iacweb |
Hace 2 years 3 months |
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The NaI resonance lines as a spectroscopic test of late-type stellar atmospheres. |
iacweb |
Hace 2 years 3 months |
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Beryllium abundances in parent stars of extrasolar planets: 16 Cygni A & B and rho (1) CANCRI |
iacweb |
Hace 2 years 3 months |
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An Optical Intermediate Dispersion Spectrograph for the GTC |
iacweb |
Hace 2 years 3 months |
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The age-mass relation for chromospherically active binaries. III. Lithium depletion in giant components |
iacweb |
Hace 2 years 3 months |
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Probing the {Na} BT I D and {K} BT I lambda 7699 resonance lines sensitivity to background opacity in late-type stars |
iacweb |
Hace 2 years 3 months |
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Optical follow-up of ROSAT discovered candidate members of the open cluster Coma Berenices |
iacweb |
Hace 2 years 3 months |
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On the potassium-rotation connection in late-type Alpha Persei stars |
iacweb |
Hace 2 years 3 months |
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Dynamic activity in the outer atmospheres of late-type stars including the sun |
iacweb |
Hace 2 years 3 months |
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Dynamic activity in the outer atmospheres of late-type stars including the Sun |
iacweb |
Hace 2 years 3 months |
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Evidence of the FIP Effect in the Coronae of Late-Type Giants |
iacweb |
Hace 2 years 3 months |
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A New Technique to Measure Magnetic Field Strength in Active Stars |
iacweb |
Hace 2 years 3 months |
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Spectral lines unaffected by instrumental polarization. 1: Theory |
iacweb |
Hace 2 years 3 months |
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Spectral lines unaffected by instrumental polarization. II. Selected lines of astrophysical interest |
iacweb |
Hace 2 years 3 months |
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Uncertainties in the determination of the Stokes parameters due to photon noise. |
iacweb |
Hace 2 years 3 months |
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Micro-structured magnetic atmospheres |
iacweb |
Hace 2 years 3 months |
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Elusive Magnetic Structures in the Sun and Solar-Type Stars |
iacweb |
Hace 2 years 3 months |
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High resolution 2D spectro-polarimetric observations of the quiet Sun in two iron lines |
iacweb |
Hace 2 years 3 months |
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Simultaneous Visible and Infrared Spectropolarimetry of a Solar Internetwork Region |
iacweb |
Hace 2 years 3 months |
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Quiet sun magnetic fields vs. polar faculae - local vs. global dynamo? |
iacweb |
Hace 2 years 3 months |
Publicación |
Physical Properties of the Solar Magnetic Photosphere under the MISMA Hypothesis. III. Sunspot at Disk Center |
iacweb |
Hace 2 years 3 months |
Publicación |
On the Sr I λ4607 Å Hanle depolarization signals in the quiet Sun |
iacweb |
Hace 2 years 3 months |
Publicación |
Magnetic flux in the inter-network quiet Sun from comparison with numerical simulations |
iacweb |
Hace 2 years 3 months |
Publicación |
A Simple Model for the Distribution of Quiet-Sun Magnetic Field Strengths |
iacweb |
Hace 2 years 3 months |
Publicación |
The dynamic magnetic quiet Sun: physical mechanisms and UV signature |
iacweb |
Hace 2 years 3 months |