OpenAlex 1.327 eser 35 yazar konusu
Çalışmalar
1.327 eser
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YÖKSİS
SJR Q1
JCR Q1
OpenAlex 78.3%
Özet henüz yok.
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YÖKSİS
SJR Q1
JCR Q1
OpenAlex 81.2%
Özet henüz yok.
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YÖKSİS
SJR Q1
JCR Q1
OpenAlex 81.2%
Özet henüz yok.
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YÖKSİS
SJR Q2
JCR Q2
OpenAlex üst %10
OpenAlex 95.9%
Özet henüz yok.
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YÖKSİS
SJR Q2
JCR Q2
OpenAlex üst %10
OpenAlex 95.9%
Özet henüz yok.
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Broadband X-ray spectra of GX 339-4 and the geometry of accreting black holes in the hard state 2008YÖKSİS SJR Q1 JCR Q1 OpenAlex üst %10 OpenAlex 96.2%
A major question in the study of black hole binaries involves our understanding of the accretion geometry when the sources are in the ``hard'' state, with an X-ray energy spectrum dominated by a hard power-law component and radio emission coming from a steady ``compact'' jet. Although the common hard state picture is…
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Shoulder terminal range eccentric antagonist concentric agonist strength ratios in overhead athletes 2006YÖKSİS SJR Q1 JCR Q1 OpenAlex 77.7%
OBJECTIVE: The agonist-antagonist strength relationship for shoulder external rotation and internal rotation was formerly described by the relatively more functional ratios of eccentric external rotator to concentric internal rotator moments, and eccentric internal rotator to concentric external rotator moments for th…
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Shoulder terminal range eccentric antagonist/concentric agonist strength ratios in overhead athletes 2006YÖKSİS SJR Q1 JCR Q1 OpenAlex 78.0%
OBJECTIVE: The agonist-antagonist strength relationship for shoulder external rotation and internal rotation was formerly described by the relatively more functional ratios of eccentric external rotator to concentric internal rotator moments, and eccentric internal rotator to concentric external rotator moments for th…
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OpenAlex üst %10
OpenAlex 98.1%
Neutron stars and black holes often reside in binaries where the accretion rate onto the compact object varies by orders of magnitude. These "X-ray transients" are observed both in outburst (when the high accretion rate makes them X-ray bright) and quiescence (when the accretion rate is very low, or potentially zero).…
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OpenAlex üst %1
OpenAlex 99.4%
Özet henüz yok.
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OpenAlex üst %10
OpenAlex 92.1%
Most black hole binaries show large changes in X-ray luminosity caused primarily by variations in mass accretion rate. An important question for understanding black hole accretion and jet production is whether the inner edge of the accretion disk recedes at low accretion rate. Measurements of the location of the inner…
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YÖKSİS
SJR Q1
JCR Q1
OpenAlex üst %10
OpenAlex 93.3%
We present new results from a multiwavelength (radio/infrared/optical/X-ray) study of the black hole X-ray binary GRO J1655-40 during its 2005 outburst. We detected, for the first time, mid-infrared emission at 24 μm from the compact jet of a black hole X-ray binary during its hard state, when the source shows emissio…
Akademisyenler
35 akademisyen
- HAYRİ ERTAN 27 yazar konusu
- EMRAH KALEMCİ 18 yazar konusu
- ABDULLAH RUHİ SOYLU 8 yazar konusu
- MURAT ÇİLLİ 8 yazar konusu
- HÜSEYİN KADOĞLU 7 yazar konusu
- İNCİ KESİLMİŞ 7 yazar konusu
- ALİ ONUR CERRAH 6 yazar konusu
- MENŞURE AYDIN AVCI 6 yazar konusu
- FATMA SÖĞÜT 5 yazar konusu
- İREM ASLAN SEYHAN 5 yazar konusu
- ERBİL HARBİLİ 4 yazar konusu
- İPEK EROĞLU KOLAYİŞ 4 yazar konusu