TR
HAT-P-19 Yıldızınının Tayfsal Analizi
Öz
Bu çalışmada ötegezegen barındıran HAT-P-19 yıldızının yüksek çözünürlüklü (R = 55000)KECK/HIRES tayfı tekrar analiz edilip temel atmosfer parametreleri ve bazı elementlerin bolluğu hesaplanmıştır.
Anahtar Kelimeler
References
- Albrecht, S., vd.: Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments. AJ. 757 (2012) 18
- Asplund, M., vd.: The Chemical Composition of the Sun. ARA&A. 47 (2009) 481--522
- Blanco-Cuaresma, S., Soubiran, C., Heiter, U., Jofre, P.: iSpec: Stellar atmospheric parameters and chemical abundances. ASCL (2014) record ascl:1409.006
- Brewer, M., vd.: pectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-search Stars. APJ. 225 (2016) 36
- Buchhave, A., vd.: An abundance of small exoplanets around stars with a wide range of metallicities. Nature. 486 (2012) 375--377
- Castelli, F., Kurucz, R. L., : New Grids of ATLAS9 Model Atmospheres. (2004) arXiv:astro-ph/0405087
- Girardi, L., vd.: Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 Msun, and from Z=0.0004 to 0.03. A&AS. bf 141 (2000) 371--383
- Guillot, T., vd.: A correlation between the heavy element content of transiting extrasolar planets and the metallicity of their parent stars. A&A. 453 (2006) 21--24
Details
Primary Language
Turkish
Subjects
Astronomical Sciences (Other)
Journal Section
Conference Paper
Publication Date
December 11, 2020
Submission Date
February 19, 2019
Acceptance Date
September 3, 2019
Published in Issue
Year 2020 Volume: 1 Number: 2