@article{abramowiczEvidenceResonanceSco2003,
	title = {Evidence for a 2:3 resonance in {Sco} {X}-1 {kHz} {QPOs}},
	volume = {404},
	issn = {0004-6361},
	shorttitle = {Evidence for a 2},
	url = {https://ui.adsabs.harvard.edu/abs/2003A&A...404L..21A/abstract},
	doi = {10.1051/0004-6361:20030737},
	abstract = {We find evidence that the two high frequency QPOs in Sco X-1 are, more often than not, approximately in the 2:3 frequency ratio familiar from studies of black hole candidates (e.g., XTE J1550-564, Remillard et al. {\textbackslash}cite\{Remillard\}). This implies that the double kHz QPO phenomenon in neutron stars has its origin in properties of strong-field gravity and has little to do with the rotation of a stellar surface or any magnetic field structure anchored in the star.},
	language = {en},
	urldate = {2023-01-08},
	journal = {Astronomy and Astrophysics},
	author = {Abramowicz, M. A. and Bulik, T. and Bursa, M. and Kluźniak, W.},
	month = jun,
	year = {2003},
	pages = {L21--L24},
}

{"_id":"hp7qLWJonr5aMDc38","bibbaseid":"abramowicz-bulik-bursa-kluniak-evidencefora23resonanceinscox1khzqpos-2003","author_short":["Abramowicz, M. A.","Bulik, T.","Bursa, M.","Kluźniak, W."],"bibdata":{"bibtype":"article","type":"article","title":"Evidence for a 2:3 resonance in Sco X-1 kHz QPOs","volume":"404","issn":"0004-6361","shorttitle":"Evidence for a 2","url":"https://ui.adsabs.harvard.edu/abs/2003A&A...404L..21A/abstract","doi":"10.1051/0004-6361:20030737","abstract":"We find evidence that the two high frequency QPOs in Sco X-1 are, more often than not, approximately in the 2:3 frequency ratio familiar from studies of black hole candidates (e.g., XTE J1550-564, Remillard et al. \\cite\\Remillard\\). This implies that the double kHz QPO phenomenon in neutron stars has its origin in properties of strong-field gravity and has little to do with the rotation of a stellar surface or any magnetic field structure anchored in the star.","language":"en","urldate":"2023-01-08","journal":"Astronomy and Astrophysics","author":[{"propositions":[],"lastnames":["Abramowicz"],"firstnames":["M.","A."],"suffixes":[]},{"propositions":[],"lastnames":["Bulik"],"firstnames":["T."],"suffixes":[]},{"propositions":[],"lastnames":["Bursa"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Kluźniak"],"firstnames":["W."],"suffixes":[]}],"month":"June","year":"2003","pages":"L21–L24","bibtex":"@article{abramowiczEvidenceResonanceSco2003,\n\ttitle = {Evidence for a 2:3 resonance in {Sco} {X}-1 {kHz} {QPOs}},\n\tvolume = {404},\n\tissn = {0004-6361},\n\tshorttitle = {Evidence for a 2},\n\turl = {https://ui.adsabs.harvard.edu/abs/2003A&A...404L..21A/abstract},\n\tdoi = {10.1051/0004-6361:20030737},\n\tabstract = {We find evidence that the two high frequency QPOs in Sco X-1 are, more often than not, approximately in the 2:3 frequency ratio familiar from studies of black hole candidates (e.g., XTE J1550-564, Remillard et al. {\\textbackslash}cite\\{Remillard\\}). This implies that the double kHz QPO phenomenon in neutron stars has its origin in properties of strong-field gravity and has little to do with the rotation of a stellar surface or any magnetic field structure anchored in the star.},\n\tlanguage = {en},\n\turldate = {2023-01-08},\n\tjournal = {Astronomy and Astrophysics},\n\tauthor = {Abramowicz, M. A. and Bulik, T. and Bursa, M. and Kluźniak, W.},\n\tmonth = jun,\n\tyear = {2003},\n\tpages = {L21--L24},\n}\n\n","author_short":["Abramowicz, M. A.","Bulik, T.","Bursa, M.","Kluźniak, W."],"key":"abramowiczEvidenceResonanceSco2003","id":"abramowiczEvidenceResonanceSco2003","bibbaseid":"abramowicz-bulik-bursa-kluniak-evidencefora23resonanceinscox1khzqpos-2003","role":"author","urls":{"Paper":"https://ui.adsabs.harvard.edu/abs/2003A&A...404L..21A/abstract"},"metadata":{"authorlinks":{}},"html":""},"bibtype":"article","biburl":"https://bibbase.org/zotero/valepeirano","dataSources":["ftqMNtyNjLWewoxW9"],"keywords":[],"search_terms":["evidence","resonance","sco","khz","qpos","abramowicz","bulik","bursa","kluźniak"],"title":"Evidence for a 2:3 resonance in Sco X-1 kHz QPOs","year":2003}