UBVI CCD photometry of M11 - II. New photometry and surface density profiles

Hwankyung Sung*, M. S. Bessell, Hee Won Lee, Yong Hee Kang, See Woo Lee

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    42 Citations (Scopus)

    Abstract

    Extensive UBVI CCD photometry has been obtained for the intermediate-age open cluster M11 (NGC 6705). From this new photometry we derive the cluster parameters [V0 - Mv = 11.55 ± 0.10, E(B - V) = 0.428 ± 0.027 and radius = 16 arcmin] and age (log tage = 8.4 ± 0.1). We also derive density profiles and confirm the mass segregation in M11. The slope of the mass function increases systematically with increasing radius from the centre. We also confirm the existence of main-sequence field stars having similar photometric characteristics to M11. A large population of field red giant stars is also found in the observed fields.

    Original languageEnglish
    Pages (from-to)982-1001
    Number of pages20
    JournalMonthly Notices of the Royal Astronomical Society
    Volume310
    Issue number4
    DOIs
    Publication statusPublished - 21 Dec 1999

    Fingerprint

    Dive into the research topics of 'UBVI CCD photometry of M11 - II. New photometry and surface density profiles'. Together they form a unique fingerprint.

    Cite this