Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Çetin Bolcal"'
Autor:
Pelin Otansev, Çetin Bolcal
Publikováno v:
Volume: 10, Issue: 2 332-343
Bitlis Eren Üniversitesi Fen Bilimleri Dergisi
Bitlis Eren Üniversitesi Fen Bilimleri Dergisi
Bu çalışmada, True Basic programlama dilini kullanarak gama spektrumunu analiz eden bir bilgisayar programı yazılmıştır. Program bir ana program ve bu ana programa bağlı alt programlar şeklindedir. İnteraktif olarak çalışan programın
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b40e7febbe1c1eb77a7883321df5ce3
https://doi.org/10.17798/bitlisfen.859103
https://doi.org/10.17798/bitlisfen.859103
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 288:470-500
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f80230255d083d812ff387a77e4a0ef1
https://doi.org/10.1093/mnras/288.2.470
https://doi.org/10.1093/mnras/288.2.470
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 258:270-276
Following from previous papers of this study we present elemental abundance analyses of the sharp-lined bright Am stars 15 Vul and 32 Aqr. The values derived using fine analysis techniques are found using the stellar parameters, effective temperature
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::48013cd1328d492b59b05461d68741cf
https://doi.org/10.1093/mnras/258.2.270
https://doi.org/10.1093/mnras/258.2.270
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 252:329-333
Elemental abundance analyses of the normal F dwarfs θ Cygni and ι Piscium are performed and found to be consistent with previous papers of this study. Our derived microturbulences of 1.5 and 1.0 km s −1 are slightly smaller than found by other re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a6286a55fd0f8ed0a4007b05b156044
https://doi.org/10.1093/mnras/252.3.329
https://doi.org/10.1093/mnras/252.3.329
Publikováno v:
Upper Main Sequence Stars with Anomalous Abundances ISBN: 9789401085977
Prelimary results from an optical region study of the metallic-lined star 32 Aquarii indicate Teff = 7600 K, log g = 3.10, ξ = 4.6 km s-1, and an iron abundance about one-half solar.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::62880ce68c76b981368806bd7c1cadd1
https://doi.org/10.1007/978-94-009-4714-6_71
https://doi.org/10.1007/978-94-009-4714-6_71
Publikováno v:
Publications of the Astronomical Society of the Pacific. 99:130
Two fine analyses of the A0 III star Alpha Dra were performed using the same sources of atomic data, the same spectrophotometric data, and the same model-atmospheres code, but with photographic region spectrograms obtained at two different observator
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7b7044e7610eafed0104275b0554d27c
https://doi.org/10.1086/131965
https://doi.org/10.1086/131965