IR Monitoring of the Microquasar GRS 1915+105: Detection of Orbital and Superhump Signatures
IR Monitoring of the Microquasar GRS 1915+105: Detection of Orbital and Superhump Signatures
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We present the results of seven years of K-band monitoring of the low-mass X-ray binary GRS 1915+105. Positive correlations between the infrared flux and the X-ray flux and X-ray hardness are demonstrated. Analysis of the frequency spectrum shows that the orbital period of the system is \(P_{orb}= 30.8 \pm 0.2\) days. The phase and amplitude of the...
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IR Monitoring of the Microquasar GRS 1915+105: Detection of Orbital and Superhump Signatures
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TN_cdi_proquest_journals_2090203880
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2090203880
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2331-8422
DOI
10.48550/arxiv.0610480
