1894-2020 opt-to-NIR photometry of HO Puppis

HO Puppis (HO Pup) was considered as a Be-star candidate based on its {gamma} Cassiopeiae-type light curve, but lacked spectroscopic confirmation. Using distance measured from...船尾座HO星（HO Pup）曾基于其仙后座γ型（gamma Cassiopeiae-type）光变曲线被认定为Be星候选体，但尚未获得光谱证认。研究人员利用从……测得的距离开展了相关研究。