High angular resolution mid-infrared imaging of young stars in Orion BN/KL

被引:50
作者
Greenhill, LJ
Gezari, DY
Danchi, WC
Najita, J
Monnier, JD
Tuthill, PG
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Natl Opt Astron Observ, Tucson, AZ 85719 USA
[4] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[5] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
基金
美国国家航空航天局;
关键词
infrared : stars; ISM : individual (Orion Kleinmann-Low); stars : formation; stars : pre-main-sequence;
D O I
10.1086/386544
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present Keck Long Wavelength Spectrometer images of the Orion BN/KL star-forming region obtained in the first multiwavelength study to have 0."3 - 0."5 resolution from 4.7 to 22 mum. The young stellar objects designated infrared source n and radio source I are believed to dominate the BN/KL region. We have detected extended emission from a probable accretion disk around source n but infer a stellar luminosity on the order of only 2000 L,. Although source I is believed to be more luminous, we do not detect an infrared counterpart even at the longest wavelengths. However, we resolve the close-by infrared source, IRc2, into an arc of knots similar to10(3) AU long at all wavelengths. Although the physical relation of source I to IRc2 remains ambiguous, we suggest that these sources mark a high-density core (10(7) - 10(8) pc(-3) over similar to10(3) AU) within the larger BN/KL star-forming cluster. The high density may be a consequence of the core being young and heavily embedded. We suggest that the energetics of the BN/KL region may be dominated by this cluster core rather than one or two individual sources.
引用
收藏
页码:L57 / L60
页数:4
相关论文
共 34 条
[1]  
[Anonymous], APJ
[2]  
Bertout C, 1999, ASTRON ASTROPHYS, V352, P574
[3]   SOLAR SYSTEM-SIZED CONDENSATIONS IN THE ORION NEBULA [J].
CHURCHWELL, E ;
FELLI, M ;
WOOD, DOS ;
MASSI, M .
ASTROPHYSICAL JOURNAL, 1987, 321 (01) :516-529
[4]   Binary star speckle measurements at Calar Alto. I. [J].
Docobo, JA ;
Tamazian, VS ;
Balega, YY ;
Blanco, J ;
Maximov, AF ;
Vasyuk, VA .
ASTRONOMY & ASTROPHYSICS, 2001, 366 (03) :868-872
[5]   NEAR-INFRARED IMAGING OF THE BECKLIN-NEUGEBAUER-IRC2 REGION IN ORION WITH SUBARCSECOND RESOLUTION [J].
DOUGADOS, C ;
LENA, P ;
RIDGWAY, ST ;
CHRISTOU, JC ;
PROBST, RG .
ASTROPHYSICAL JOURNAL, 1993, 406 (01) :112-121
[6]   X-ray emitting young stars in the Orion Nebula [J].
Feigelson, ED ;
Broos, P ;
Gaffney, JA ;
Garmire, G ;
Hillenbrand, LA ;
Pravdo, SH ;
Townsley, L ;
Tsuboi, Y .
ASTROPHYSICAL JOURNAL, 2002, 574 (01) :258-292
[7]   Massive stars: Their environment and formation [J].
Garay, G ;
Lizano, S .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1999, 111 (763) :1049-1087
[8]   THE ORION MOLECULAR CLOUD AND STAR-FORMING REGION [J].
GENZEL, R ;
STUTZKI, J .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1989, 27 :41-85
[9]   Mid-infrared imaging of Orion BN/KL. II. Luminosity sources, extinction distribution, and the nature of IRc2 [J].
Gezari, DY ;
Backman, DE ;
Werner, MW .
ASTROPHYSICAL JOURNAL, 1998, 509 (01) :283-298
[10]   MIDINFRARED IMAGING OF ORION BN/KL - ASTROMETRY OF IRC2 AND THE SIO MASER [J].
GEZARI, DY .
ASTROPHYSICAL JOURNAL, 1992, 396 (01) :L43-L47