Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Elmaslı, Aslı"'
We performed spectroscopic and photometric analyses on the early B-type LP Ori young stellar object located in the Orion Nebula. The high-resolution spectra of LP Ori was obtained at the Ankara University Kreiken Observatory in 2023, while all spectr
Externí odkaz:
http://arxiv.org/abs/2403.01989
The existence of an additional body around a binary system can be detected by the help of the light-travel time effect. Due to the motions of binary and the companion stars around the common mass center of the ternary system, the light-time effect pr
Externí odkaz:
http://arxiv.org/abs/1808.07920
Publikováno v:
IJRST, 2017, Vol. No. 7, Issue No. III, Jul-Sep, e-ISSN: 2249-0604, p-ISSN: 2454-180X
We present the more refined abundances of elements (C, O, Na, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Mn, Fe, Ni, Zn, Sr, Y, Zr and Ba) determined using the computationally intensive ATLAS12 atmosphere model for the metallic-line stars Pi Dra and HR 7545. We
Externí odkaz:
http://arxiv.org/abs/1710.09570
Autor:
Elmasli, Asli, Caliskan, Seyma, Kilicoglu, Tolgahan, Unal, Kubraozge, Nasolo, Yahya, Albayrak, Berahitdin
The atmospheric parameters and chemical abundances of two neglected A-type stars, 28 Peg and HD 202240, were derived using high resolution spectra obtained at the TUBITAK National Observatory. We determined the photospheric abundances of eleven eleme
Externí odkaz:
http://arxiv.org/abs/1507.00475
Publikováno v:
Astronomische Nachrichten; Jun2024, Vol. 345 Issue 5, p1-16, 16p
Publikováno v:
In New Astronomy July 2018 62:15-19
Akademický článek
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Autor:
Elmaslı, Aslı, Çalışkan, Şeyma, Kılıçoğlu, Tolgahan, Ünal, Kübraözge, Nasolo, Yahya, Albayrak, Berahitdin
Publikováno v:
In New Astronomy January 2016 42:38-41
Autor:
Elmaslı, Aslı, Ünal, Kübra Özge
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Oct2023, Vol. 524 Issue 4, p6285-6294, 10p
Autor:
Çalışkan, Şeyma, Kılıçoğlu, Tolgahan, Elmaslı, Aslı, Nasolo, Yahya, Avcı, Zeynep, Albayrak, Berahitdin
Publikováno v:
In New Astronomy January 2015 34:6-10