The Chemical Composition of the Sun
The solar chemical composition is an important ingredient in our understanding of the formation, structure, and evolution of both the Sun and our Solar System. Furthermore, it i...
Publications
View All<i>Gaia</i> Data Release 2
Context. We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability,...
<i>Gaia</i>Early Data Release 3
Context. We present the early installment of the third Gaia data release, Gaia EDR3, consisting of astrometry and photometry for 1.8 billion sources brighter than magnitude 21, ...
Line formation in solar granulation
The solar photospheric oxygen abundance has been determined from [O I], O I, OH vibration-rotation and OH pure rotation lines by means of a realistic time-dependent, 3D, hydrody...
Line formation in solar granulation
The solar photospheric carbon abundance has been determined from [C i], C i, CH vibration-rotation, CH A-X electronic and C2 Swan electronic lines by means of a time-dependent, ...
Affiliated Researchers
Institution Info
- Type
- facility
- Country
- BE
- Publications
- 5
- Citations
- 21,445
External Links
Identifiers
- ROR
- https://ror.org/00hjks330