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Titolo:
Submillimeter maps of small young clusters in three large globules
Autore:
Huard, TL; Weintraub, DA; Sandell, G;
Indirizzi:
Vanderbilt Univ, Dept Phys & Astron, Stn B, Nashville, TN 37235 USA Vanderbilt Univ Nashville TN USA 37235 on, Stn B, Nashville, TN 37235 USA Natl Radio Astron Observ, Green Bank, WV 24944 USA Natl Radio Astron Observ Green Bank WV USA 24944 Green Bank, WV 24944 USA
Titolo Testata:
ASTRONOMY AND ASTROPHYSICS
fascicolo: 2, volume: 362, anno: 2000,
pagine: 635 - 645
SICI:
0004-6361(200010)362:2<635:SMOSYC>2.0.ZU;2-9
Fonte:
ISI
Lingua:
ENG
Soggetto:
ORION NEBULA CLUSTER; T-TAURI STARS; BOK GLOBULES; STELLAR OBJECTS; HIGH-RESOLUTION; DUST EMISSION; NGC-1333; CLOUD; CORES; L810;
Keywords:
stars : formation; stars : pre-main sequence; ISM : clouds; ISM : dust, extinction; ISM : individual objects : CB34 L810;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
60
Recensione:
Indirizzi per estratti:
Indirizzo: Huard, TL Vanderbilt Univ, Dept Phys & Astron, Stn B, POB 1807, Nashville,TN 37235 USA Vanderbilt Univ POB 1807 Nashville TN USA 37235 le, TN 37235 USA
Citazione:
T.L. Huard et al., "Submillimeter maps of small young clusters in three large globules", ASTRON ASTR, 362(2), 2000, pp. 635-645

Abstract

We present submillimeter maps of regions within three large globules, CB 3, CB 34, and L 810. Our maps are centered on three IRAS sources, each of which is associated with a small cluster of near-infrared young stellar objects (YSOs) as seen from deep optical and/or near-infrared observations. We have detected submillimeter sources associated with the YSO clusters. The submillimeter emission appears to be primarily from small clusters of protostars rather than from the sources previously detected in the near-infrared. This result suggests that these large globules are currently adding protostars to these clusters. Thus, star formation within each of these large globules appears to be a continuous process rather than a single, isolated event.

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Documento generato il 26/05/13 alle ore 03:25:19