2001A&A...368L..34C

Query : 2001A&A...368L..34C

2001A&A...368L..34C - Astronomy and Astrophysics, volume 368, L34-37 (2001/3-4)

SiO emission from a huge, detached shell in IRC+10420.

CASTRO-CARRIZO A., LUCAS R., BUJARRABAL V., COLOMER F. and ALCOLEA J.

Abstract (from CDS):

We present observations of the v=0 J=2-1 thermal emission of SiO from the very luminous evolved star IRC+10420, performed with the Plateau de Bure interferometer. Our high-resolution maps show that the emission comes from a huge hollow shell, with a typical radius of ∼1017cm, that is expanding at ∼35km/s. This surprising result is strengthened by model fitting of the flux distribution, that explains the observations assuming that the width of the shell is not larger than half its typical radius. The origin of this feature is discussed.

Abstract Copyright: ∼

Journal keyword(s): stars: individual: IRC+10420 - (stars:) circumstellar matter - stars: AGB y post-AGB - radio lines: stars - stars: mass-loss

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 3C 273 BLL 12 29 06.6998257176 +02 03 08.597629980   13.05 14.830 14.11   ~ 5798 1
2 ICRF J192559.6+210626 BLL 19 25 59.60535459 +21 06 26.1620257           ~ 203 1
3 IRC +10420 pA* 19 26 48.0979492536 +11 21 16.758531216   13.98 11.66     F8Ia+e 477 0

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