2008
			
	    
	
	
    Distribution of Kilohertz QPO Frequencies and Their Ratios in the Atoll Source 4U 1636-53
ABRAMOWICZ, Marek; Pavel BAKALA; Zdeněk STUCHLÍK a Gabriel TÖRÖKZákladní údaje
Originální název
Distribution of Kilohertz QPO Frequencies and Their Ratios in the Atoll Source 4U 1636-53
	Název anglicky
Distribution of Kilohertz QPO Frequencies and Their Ratios in the Atoll Source 4U 1636-53
		Autoři
Vydání
 Acta Astronomica, PL - Polská republika, 2008, 0001-5237
			Další údaje
Typ výsledku
Článek v odborném periodiku
		Obor
10308 Astronomy
		Utajení
není předmětem státního či obchodního tajemství
		Impakt faktor
Impact factor: 1.778
			Organizační jednotka
Fyzikální ústav v Opavě
			UT WoS
000255383600002
		EID Scopus
2-s2.0-44149086204
		Klíčová slova anglicky
QPO, frequency ratio
		Štítky
Příznaky
Mezinárodní význam, Recenzováno
		Návaznosti
LC06014, projekt VaV. MSM4781305903, záměr. 
			
				
				Změněno: 6. 4. 2021 13:31, Mgr. Pavlína Jalůvková
				
		V originále
We find that the distribution of the ratio of actually observed pairs of kHz QPO frequencies is peaked close to the 3/2 value, and possibly also close to the 5/4 ratio. To resolve the apparent contradiction between the two studies, we examine in detail the frequency distributions of the lower kHz QPO and the upper kHz QPO detected in our data set. We demonstrate that for each of the two kHz QPOs (the lower or the upper), the frequency distribution in all detections of a QPO differs from the distributionof frequency of the same QPO in the subset of observations where both the kHz QPOs are detected. We conclude that detections of individual QPOs alone should not be used for calculation of the distribution of the frequency ratios.
				Anglicky
We find that the distribution of the ratio of actually observed pairs of kHz QPO frequencies is peaked close to the 3/2 value, and possibly also close to the 5/4 ratio. To resolve the apparent contradiction between the two studies, we examine in detail the frequency distributions of the lower kHz QPO and the upper kHz QPO detected in our data set. We demonstrate that for each of the two kHz QPOs (the lower or the upper), the frequency distribution in all detections of a QPO differs from the distributionof frequency of the same QPO in the subset of observations where both the kHz QPOs are detected. We conclude that detections of individual QPOs alone should not be used for calculation of the distribution of the frequency ratios.