Tallenna
Progress in Stellar Spectral Line Formation Theory
Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars.
- Toimittaja
- J.E. Beckman, L. Crivellari
- Painos
- Softcover reprint of the original 1st ed. 1985
- ISBN
- 9789401088701
- Kieli
- englanti
- Paino
- 310 grammaa
- Julkaisupäivä
- 10.11.2011
- Kustantaja
- Springer
- Sivumäärä
- 464
