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- W3173485142 abstract "Young open clusters are ideal laboratories to understand star formation process. We present deep UBV I and Halpha photometry for the young open cluster IC 1590 in the center of the H II region NGC 281. Early-type members are selected from UBV photometric diagrams, and low-mass pre-main sequence (PMS) members are identified by using Halpha photometry. In addition, the published X-ray source list and Gaia astrometric data are also used to isolate probable members. A total of 408 stars are selected as members. The mean reddening obtained from early-type members is 1 M_sun). The signature of mass segregation is detected from the difference in the slopes of the initial mass functions for the inner (r < 2.'5) and outer region of this cluster. We finally discuss the star formation history in NGC 281." @default.
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- W3173485142 date "2021-06-29" @default.
- W3173485142 modified "2023-10-16" @default.
- W3173485142 title "The Sejong Open Cluster Survey (SOS). VII. A Photometric Study of the Young Open Cluster IC 1590" @default.
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