The Pre–Main-Sequence Stars and Initial Mass Function of NGC 2264
Byeong-Gon ParkBohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory, Youngcheon, Kyungpook 770-820, KoreaHwankyung SungBohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory, Youngcheon, Kyungpook 770-820, KoreaM. S. BessellResearch School of Astronomy and Astrophysics, Australian National University, Private Bag, Weston Creek, ACT 2611, AustraliaYong Hee KangDepartment of Earth Science Education, Kyungpook National University, Taegu 702-701 Korea
2000en
ABI
Аннотация
UBVRI and Hα CCD photometry has been performed in the southern region of NGC 2264 around the Cone Nebula. A nearly complete list of pre-main-sequence (PMS) members in the cluster has been made from the compilation of Hα emission stars identified in this
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
3 та иқтибос0 та фойдаланилган манба