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| 1 | A critical view on the performance and design of combined cooled ceiling and displacement ventilation systems显示文摘 | ATILA N JELENA S | 2001 | Energy and Buildings2001，，： | 1 |
| 2 | A method of streamflow drought a- nalysis 显示文摘 | EMIR Z ATILA S | 1987 | Water Resources Research1987，23，1： | 1 |
| 3 | Incarcerated inferior lumbar (Petit's) hernia显示文摘 | Astarcioglu H S(o)kmen S Atila K | 2003 | Hernia2003，7，3： | 1 |
| 4 | A method of streamflow drought analysis 显示文摘 | Emir Z Atila S | 1987 | Water Resources Research1987，23，1： | 1 |
| 5 | A critical review on the performance and design of combined cooled ceiling and displacement ventilation显示文摘 | Atila N Jelena S | 2002 | Energy and Buildings2002，34，5： | 1 |
| 6 | A Critical Review on the Performance and Design of Combined Cooled Ceiling mad Displacement Ventilation Systems显示文摘 | Jelena S | 2002 | Ener gy and Buildings2002，34，： | 1 |
| 7 | Prosthetic repair of a- cutely incarcerated groin hernias: a prospective clinical observa- tional cohort study显示文摘 | ATILA K GULER S INAL A | 2010 | Langenbeck''s Archives of Surgery2010，395，5： | 1 |
| 8 | Prosthetic repair of acutely incar?cerated groin hernias: a prospective clinical observational cohort study显示文摘 | Atila K GuIer S Inal A | 2010 | Langenbecks Arch Surg2010，395，5： | 1 |
| 9 | A critical review on the performance and design of combined cooled ceiling and displacement ventilation systems显示文摘 | Atila N Jelena S | | 0，，05： | 1 |
| 10 | A critical review on the performance and design of combined cooled ceiling and displacement ventilation systems 显示文摘 | Atila N Jelena S | 2002 | Energy and Buildings2002，34，5： | 1 |
| 11 | Prosthetic repair of acutely incarcerated groin hernias: a prospective clinical observational cohort study显示文摘 | Atila K Guler S Inal A | 2010 | Langenbecks Arch Surg2010，395，5： | 1 |
| 12 | Prosthetic repair of acutely incarcerated groin hernias:a prospective clinicat observational cohort study显示文摘 | Atila K Guler S Inal A et aI | 2010 | Langenbecks Arch Surg2010，595，5： | 1 |
| 13 | Prosthetic repair of acutely incarcerated groin hernias: a prospective clinical observational cohort study显示文摘 | Atila K Guler S Inal A | 2010 | Langenbecks Arch Surg2010，395，5： | 1 |
| 14 | Prosthetic repair of acutely incarcerated groin hernias:a prospective clinical observational cohort study显示文摘 | Atila K Guler S Inal A | 2010 | Langenbecks Arch Surg2010，395，5： | 1 |
| 15 | Prosthetic repair of acutely incar- cerated groin hernias: a prospective clinical observational cohort study显示文摘 | Atila K GuleT S Inal A | 2010 | Langenbecks Arch Surg2010，395，5： | 1 |
| 16 | What is the role of the abdominal perfusion pressure for subclinical hepatic dysfunction in laparoscopic cholecystectomy显示文摘 | Atila K Terzi C Ozkardesler S | | 0，，01： | 1 |
| 17 | BVRI photometric observations,light curve solutions and orbital period analysis of BF Pav显示文摘A new ephemeris,period change analysis and light curve modeling of the W UMa-type eclipsing binary BF Pav are presented in this study.Light curves of the system taken in BVRI filters from two observatories,in Australia and Argentina,were modeled using the Wilson-Devinney code.The results of this analysis demonstrate that BF Pav is a contact binary system with a photometric mass ratio q=1.460 ± 0.014,a fillout factor f=12.5%,an inclination of 87.97 ± 0.45 deg and a cold spot on the secondary component.By applying the distance modulus formula,the distance of BF Pav was calculated to be d=268 ± 18 pc which is in good agreement with the Gaia EDR3 distance.We obtain an orbital period increase at a rate of 0.142 s century-1 due to a quadratic trend in the O-C diagram.Also,an alternative sudden period jump probably occurred which could be interpreted as a rapid mass transfer from the lower mass star to its companion of about ΔM=2.45 × 10-6 M⊙.Furthermore,there is an oscillatory behavior with a period of 18.3±0.3 yr.Since BF Pav does not seem to have significant magnetic activity,this behavior could be interpreted as the light-time effect caused by an undetected third body in this system.In this case,the probability for the third body to be a low mass star with M≥ 0.075 M⊙or a brown dwarf is 5.4% and 94.6% respectively.If we assume i’=90°,a3=8.04±0.33 AU.The mass of the secondary component was also determined following two different methods which result close to each other. | Atila Poro Fahri Alicavus Eduardo Fernández-Lajús Fatemeh Davoudi PegahSadat MirshafieKhozani Mark G.Blackford Edwin Budding Behjat Zarei Jalalabadi Jabar Rahimi Farzaneh Ahangarani Farahani | 2021 | Research in Astronomy and Astrophysics2021，21，8： | 0 |
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