Measurement of Dependence of Microlensing Planet Frequency on The Host Star Mass and Galactocentric...
Measurement of Dependence of Microlensing Planet Frequency on The Host Star Mass and Galactocentric Distance by using a Galactic Model
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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 measure the dependence of planet frequency on host star mass, \(M_{\rm L}\), and distance from the Galactic center, \(R_{\rm L}\), using a sample of planets discovered by gravitational microlensing. We compare the two-dimensional distribution of the lens-source proper motion, \(\mu_{\rm rel}\), and the Einstein radius crossing time, \(t_{\rm E}\...
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Measurement of Dependence of Microlensing Planet Frequency on The Host Star Mass and Galactocentric Distance by using a Galactic Model
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TN_cdi_proquest_journals_2937452578
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2937452578
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2331-8422
