@article{
 title = { X‐Ray Properties of Young Stellar Objects in OMC‐2 and OMC‐3 from the Chandra X‐Ray Observatory },
 type = {article},
 year = {2002},
 identifiers = {[object Object]},
 pages = {974-981},
 volume = {566},
 websites = {http://stacks.iop.org/0004-637X/566/i=2/a=974},
 month = {2},
 publisher = {IOP Publishing},
 day = {20},
 id = {e1434f69-4469-3d1a-afb5-a8d9c2589ae3},
 created = {2019-11-05T08:27:53.442Z},
 accessed = {2018-01-30},
 file_attached = {true},
 profile_id = {ec4888e4-cd9f-3ee0-90a1-39a024d1537d},
 last_modified = {2022-07-15T21:49:05.284Z},
 read = {true},
 starred = {false},
 authored = {true},
 confirmed = {true},
 hidden = {false},
 citation_key = {tsujimoto02a},
 source_type = {article},
 folder_uuids = {9989056f-58f0-4daf-a99f-4779f0cdd416,5a859072-32ae-4559-8859-863b99a8e32c},
 private_publication = {false},
 abstract = {We report X-ray results of the Chandra observation of Orion Molecular Cloud 2 and 3. A deep exposure of \sim 100 ksec detects \sim 400 X-ray sources in the field of view of the ACIS array, providing one of the largest X-ray catalogs in a star forming region. Coherent studies of the source detection, time variability, and energy spectra are performed. We classify the X-ray sources into class I, class II, and class III+MS based on the J, H, and K-band colors of their near infrared counterparts and discuss the X-ray properties (temperature, absorption, and time variability) along these evolutionary phases.},
 bibtype = {article},
 author = {Tsujimoto, Masahiro and Koyama, Katsuji and Tsuboi, Yohko and Goto, Miwa and Kobayashi, Naoto},
 journal = {The Astrophysical Journal},
 number = {2}
}

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