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Baris 308: \| {{nowrap\|[[HD 13189]]}}<ref name=XPE13189-2010-11-28/> \| {{Solar mass\|link=y\|4.5±2.5}}<ref name=XPE13189-2010-11-28/> \| Margin of error means the star [[NGC 4349-127]] with a stellar mass of {{Solar mass\|3.9}} is potentially the most massive known planet-harboring star.<ref>{{cite encyclopedia \| title=Notes for planet NGC 4349-127 b \| encyclopedia=The Extrasolar Planets Encyclopaedia \| url=http://exoplanet.eu/catalog/ngc_4349_no_127_b/\| accessdate=2017-08-28\| archive-date=2017-08-28\| archive-url=https://web.archive.org/web/20170828225846/http://exoplanet.eu/catalog/ngc_4349_no_127_b/\| dead-url=yes}}</ref> [[Mirfak]] ({{Solar mass\|8.4}} hypothetically has one planet, but this remains unproven. The extremely massive stars R66 ({{Solar mass\|70}}) and R126 ({{Solar mass\|30}}) have protoplanetary disks but it is unknown if there are planets in this system.

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