1996A&A...315L.293S

Query : 1996A&A...315L.293S

1996A&A...315L.293S - Astronomy and Astrophysics, volume 315L293-296 (1996/11-2)

LWS observations of the bright rimmed globule IC 1396N.

SARACENO P., CECCARELLI C., CLEGG P., CORREIA C., DI GIORGIO A., GIANNINI T., GRIFFIN M., LORENZETTI D., MOLINARI S., NGUYEN-Q-RIEU, NISINI B., RADICCHI A., SPINOGLIO L., TOMMASI E., WHITE G.J., ADE P.A.R., ANDRE P., ARMAND C., BARLOW M.J., BURGDORF M., CAUX E., CERULLI P., FISCHER J., FURNISS I., GLENCROSS W., GRY C., KING K.J., LIM T., LISEAU R., MINCHIN N., NAYLOR D., TEXIER D., ORFEI R., PALLA F., SIDHER S., SMITH H.A., SWINYARD B., TRAMS N. and UNGER S.

Abstract (from CDS):

We present the first far-infrared spectrum of the IRAS source associated with IC 1396N, located in the HII region IC 1396 together with submillimeter and millimeter photometry. A rich spectrum of CO, OH, and H2O lines are detected in the ISO-LWS spectrum, indicative of a warm, dense region, probably shock excited, around the source. Among the fine structure lines, [OIII] and [NIII] are also detected and can be explained by the presence of the O6 star HD206267 approximately 16pc away. The far infrared and submillimeter spectral energy distribution is fitted with a model assuming spherical grey-bodies with a radial power law of density and temperature. An accurate measure of the bolometric luminosity and an estimate of the total envelope mass are obtained.

Abstract Copyright: ∼

Journal keyword(s): stars: formation - ISM: jets and outflows - ISM: individual objects: IC 1396N - infrared: ISM:lines

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 IC 1396 OpC 21 38 51.4 +57 31 52           ~ 523 1
2 HD 206267 Y*O 21 38 57.6195772032 +57 29 20.554016280 5.09 5.83 5.62   5.56 O6.0V((f))+O9:V 520 0
3 [BGE2002] BIMA 2 Y*O 21 40 42.36 +58 16 09.7           ~ 123 0
4 NAME IC 1396 North CGb 21 40 42.6537 +58 16 01.882           ~ 193 1
5 Ass Cep OB 2 As* 21 51 +60.0           ~ 303 0

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