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THE INITIAL MASS FUNCTION AND YOUNG BROWN DWARF CANDIDATES IN NGC 2264. III. PHOTOMETRIC DATA

Hwankyung SungDepartment of Astronomy and Space Science, Sejong University, Kunja‐dong 98, Kwangjin‐gu, Seoul 143‐747, KoreaM. S. BessellResearch School of Astronomy and Astrophysics, Australian National University, MSO, Cotter Road, Weston, ACT 2611, AustraliaMoo‐Young ChunOptical Astronomy Division, Korea Astronomy and Space Science Institute, Whaam-dong 61-1, Yusung-gu, Taejeon 305-348, KoreaR. KarimovUlugh Beg Astronomical Institute, 33 Astronomical Street, Tashkent 700052, Uzbekistan,M. IbrahimovUlugh Beg Astronomical Institute, 33 Astronomical Street, Tashkent 700052, Uzbekistan,

The Astronomical Journaljournal2008en

ABI

Annotatsiya

We have performed deep wide-field CCD photometry of the young open cluster NGC 2264 to study the extent of star-forming regions (SFRs) and the shape of the initial mass function. In this paper, we present VRI and Hα photometry for more than 67,000 stars.

Mavzular

Astrophysics and Star Formation Studies Stellar, planetary, and galactic studies Astro and Planetary Science

Identifikatorlar

DOI: 10.1088/0004-6256/135/2/441

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