A Settlement Analysis at Byzantine Komana through Excavation Survey and GIS Data

Date

2014-04-26

Author

Erciyas, Deniz Burcu
Süzen, Mehmet Lütfi

Metadata

Show full item record

Item Usage Stats

22
views

0
downloads

URI

https://hdl.handle.net/11511/74909

Collections

Unverified, Conference / Seminar

Suggestions

OpenMETU
Core

A qualitative and quantitative assesment of soil acidification due to a thermal power plant:a case study Kılıç, Başak; Soyupak, Selçuk; Department of Environmental Engineering (1992)
A study of animal husbandry at Şapinuva through animal remains, 86Sr/88Sr isotope analysis, geometric morphometrics and Hittite texts. Pişkin, Evangelia (2021-12-16) A study of animal husbandry at Şapinuva through animal remains, 86Sr/88Sr isotope analysis, geometric morphometrics and Hittite texts.E. Pişkin, A. Süel, İ. Kandemir, S. Köksal, G. Özger, G. Durdu, M. Aydın, S. Gerçek.(Aygül hocam, Murat ve Semih isimleri alfabetik sıra ile koydum. Ne düşünüyorsun? Bu doğru mu? Sıralamayı değiştirmek istiyorsanız lütfen yapın)Animal husbandry and agriculture were central to the economic success of the Hittite state. Numerous laws were issued to regulate every detail...
A high-resolution, multi-isotopic study of mantle heterogeneity beneath the southeast Indian Ridge: Preliminary Pb and Hf results Hanan, Bb; Blichert-Toft, J; Sayıt, Kaan; Agranier, A; Hemond, C; Briais, A; Maia,, M; Graham, D; Albarede, F (2011-08-14)
A Comparative Reliability Analysis for Draglines in Turkey Demirel, Nuray; Kestel, Sevtap Ayşe (2012-11-30)
A photometric-spectroscopic analysis and the evolutionary status of the Algol-type binary U Coronae Borealis Yerli, Sinan Kaan; Zola, S; Smith, RC; Tovmassian, G (Oxford University Press (OUP), 2003-07-11) The prime purposes of this study are to obtain reliable orbital parameters for the Algol-type binary U Coronae Borealis (U CrB) and to explain the evolutionary status of this system. All observations of the primary star's radial velocity are consistent with the value K(1) = 58.6 +/- 2.0 km s(-1). Measurements of the radial velocity of the secondary component give K(2) = 185.2 +/- 5.0 km s(-1). Using the photometrically determined inclination of 78.7 +/- 0.3, the masses of the two stars are therefore deduced...

Citation Formats

D. B. Erciyas and M. L. Süzen, “A Settlement Analysis at Byzantine Komana through Excavation Survey and GIS Data,” 2014, Accessed: 00, 2021. [Online]. Available: https://hdl.handle.net/11511/74909.