Artikel
Open Access
Chemical Composition of the RS CVN-Type Star 29 Draconis
-
G. Barisevičius
Veröffentlicht/Copyright:
19. April 2017
Received: 2010-10-2
Accepted: 2010-11-5
Published Online: 2017-4-19
Published in Print: 2010-12-1
© 2017
Artikel in diesem Heft
- On the Optical Spectrum of Mu Cephei
- Chemical Composition of the RS CVN-Type Star 29 Draconis
- Extinctions and Distances to Dark Clouds from 2MASS, MegaCam and IPHAS Surveys: LDN 1525 in the Direction of the Aur OB1 Association
- Star Classification Possibilities with the Gaia Spectrophotometers. II. A Method for Empirical Decontamination of the BP/RP Spectra
- Wide Field Multicolor CCD Photometry in the Vicinity of the Open Cluster King 7
- High Velocity Spectroscopic Binary Orbits from Photoelectric Radial Velocities: BD+20 5152, a Possible Triple System
- The Apollo Group Asteroid 2008 OS9: Discovery, Orbit, Rotation and the Yarkovsky/YORP Effects
- Changes in the Cloud Belts of Jupiter, 1630–1664, as Reported in the 1665 Astronomia Reformata of Giovanni Battista Riccioli
Schlagwörter für diesen Artikel
stars;
RS CVn binaries;
abundances stars;
individual (29 Draconis = HD 160538))
Creative Commons
BY-NC-ND 4.0
Artikel in diesem Heft
- On the Optical Spectrum of Mu Cephei
- Chemical Composition of the RS CVN-Type Star 29 Draconis
- Extinctions and Distances to Dark Clouds from 2MASS, MegaCam and IPHAS Surveys: LDN 1525 in the Direction of the Aur OB1 Association
- Star Classification Possibilities with the Gaia Spectrophotometers. II. A Method for Empirical Decontamination of the BP/RP Spectra
- Wide Field Multicolor CCD Photometry in the Vicinity of the Open Cluster King 7
- High Velocity Spectroscopic Binary Orbits from Photoelectric Radial Velocities: BD+20 5152, a Possible Triple System
- The Apollo Group Asteroid 2008 OS9: Discovery, Orbit, Rotation and the Yarkovsky/YORP Effects
- Changes in the Cloud Belts of Jupiter, 1630–1664, as Reported in the 1665 Astronomia Reformata of Giovanni Battista Riccioli
