Corpus ID: 111932486

FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)

@inproceedings{Ramadhan2015FOTOMETRIGB,
  title={FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)},
  author={Fajar Ramadhan and Rhorom Priyatikanto and J. A. Utama},
  year={2015}
}
Gugus bintang terbuka M67 merupakan salah satu gugus bintang paling tua di Galaksi Bima Sakti dan merupakan warisan masa lampau yang masih ada hingga kini. Gugus bintang terbuka M67 juga merupakan gugus bintang dengan anggota terbanyak dengan observed member sekitar 649 bintang (Sanders, 1989). Studi tentang gugus bintang terutama gugus bintang tua bertujuan untuk memahami hal-hal seperti struktur galaksi, komposisi kimia, populasi bintang, evolusi dinamis dan proses pembentukan bintang-bintang… Expand

References

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Close binary and other variable stars in the solar-age Galactic open cluster M 67
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M 67 (NGC 2682). About 3600 frames spread over 28 nights were obtained with the 1.5 m Russian-Turkish and 1.2Expand
DEEP 2MASS PHOTOMETRY OF M67 AND CALIBRATION OF THE MAIN-SEQUENCE J - KS COLOR DIFFERENCE AS AN AGE INDICATOR
We present an analysis of Two Micron All Sky Survey (2MASS) calibration photometry of the old open cluster M67 (NGC 2682). The proper-motion-cleaned color-magnitude diagram (CMD) resulting from theseExpand
Examining the M67 Classification as an Open Cluster
The cluster M67 (= NGC 2682) in Cancer is a rich stellar cluster, usually classified as an open cluster. Using our own observations with the 0.4 m telescope, we show that M67 is a tight group ofExpand
CCD photometry of the old open cluster M67
We present a CCD photometric survey of the central one-half degree of the old open cluster, M67, in U, B, V, and I colors to magnitude V=20. Extensive comparison of our photometry with otherExpand