| (82) HR 6819 is a binary system with no black hole. Revisiting the source with infrared interferometry and optical integral field spectroscopy
- Frost, A. J. et al
- published in Astronomy & Astrophysics, 659 issue L3, pp. 12 (2022)
- SCART-2023-0074
|
| (79) The Belgian Repository of Fundamental Atomic Data and Stellar Spectra (BRASS)
- Lobel, Alex et al
- published in Atoms, 7 issue 4, pp. 105 (11 pages) (2019)
- SCART-2020-0069
|
| (79) Influence of a uniform coronal magnetic field on solar p modes
- Vanlommel, P. et al
- submitted to ESA SP Series, 506 (2002)
- SIDCimport-4
|
| (77) Automated Detection of Accelerating Solar Eruptions using Parabolic Hough Transform
- Patel, Ritesh et al
- published in Solar Physics (2020)
- SCART-2021-0041
|
| (76) Signatures of Slow Solar Wind Streams from Active Regions in the Inner Corona
- Slemzin, V.A. et al
- published in Solar Physics, 286, pp. 157--184 (2013)
- SIDCimport-527
| |