2004BaltA..13..415L

Query : 2004BaltA..13..415L

2004BaltA..13..415L - Baltic Astronomy, 13, 415-418 (2004/August-0)

Physical conditions of high-luminosity star-forming regions observed by ISO-LWS.

LEEKS S.J., SPINOGLIO L., MONTINARO L., BENEDETTINI M. and VITI S.

Abstract (from CDS):

We present here the results obtained with the Infrared Space Observatory's Long Wavelength Spectrometer on a sample of high-luminosity star forming regions, characterized by the presence of strong far ultraviolet stellar fields causing atomic ionization. We show how photoionization models can explain the observed fine structure line luminosities and where other components, such as photodissociation emission and shock excitation by outflows, have to be included to account for the observed spectra.

Abstract Copyright: ∼

Journal keyword(s): stars: pre-main-sequence, formation - ISM: H II regions - ISM: jets and outflows - ISM: lines and bands

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 NGC 281 HII 00 52 25.1 +56 33 54           ~ 251 1
2 RAFGL 2046 HII 18 00 32.1 -24 04 03           ~ 380 0
3 RAFGL 2059 Y*O 18 04 53.1586569336 -24 26 41.642012796 19.905 21.910 18.914   14.078 ~ 146 0
4 2MASS J23133024+6130103 Y*? 23 13 30.2430274824 +61 30 10.334305152           O9.5V+B0.5V 31 0
5 NGC 7538 OpC 23 13 37 +61 30.0           ~ 920 1

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