2006ApJ...640..353M


Query : 2006ApJ...640..353M

2006ApJ...640..353M - Astrophys. J., 640, 353-359 (2006/March-3)

Subarcsecond mid-infrared imaging of dust in the bipolar nebula Hen 3-401.

MUTHUMARIAPPAN C., KWOK S. and VOLK K.

Abstract (from CDS):

We present high-resolution, nearly diffraction-limited narrow- and broadband mid-IR images of bipolar reflection nebula Hen 3-401. The deconvolved images yield a pixel-limited spatial resolution of 0".09, demonstrating the superior imaging quality of the Gemini telescope. The infrared image of Hen 3-401 consists of a prominent core region of size 1" and extended emissions along the walls of the bipolar lobes. We find that the distribution of aromatic infrared band (AIB) emission is different from that of the continuum emission and that the star has undergone multiple ejection of the AIB emission feature carrier at the end stages of its evolution. From the observed temperature gradient in the core, we suggest that the core has a flared disk geometry.

Abstract Copyright: ∼

Journal keyword(s): ISM: Planetary Nebulae: General - Stars: AGB and Post-AGB - Stars: Emission-Line, Be

CDS comments: Parag. 3.1 : IRAS Z02229+6202 is a misprint for IRAS Z02229+6208

Simbad objects: 9

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Number of rows : 9
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 IRAS Z02229+6208 pA* 02 26 41.7882689568 +62 21 21.981286008   14.69 12.00 11.16 8.92 G8-K0_0-Ia: 65 0
2 * alf CMa SB* 06 45 08.91728 -16 42 58.0171 -1.51 -1.46 -1.46 -1.46 -1.43 A0mA1Va 1610 0
3 HD 56126 pA* 07 16 10.2590823192 +09 59 47.954735376   9.20 8.32     F0/5Ia 330 0
4 THA 35-II-27 PN 10 19 32.501 -60 13 29.48     12.5     B:Ie 90 0
5 WRAY 16-147 Sy* 14 11 52.0604355768 -51 26 24.187122024     14.20     ~ 240 1
6 PN Mz 3 PN 16 17 13.3915382496 -51 59 10.711893480   10.8 14.00     O9.5 359 0
7 PN M 2-9 PN 17 05 37.96152 -10 08 32.5068           ~ 532 0
8 IRAS 17106-3046 pA* 17 13 51.7976155656 -30 49 40.722991968       15.070   F5I 34 0
9 Min 1-92 pA* 19 36 18.9295687968 +29 32 49.785288144 12.13 12.35 11.75 11.54   B0.5IV[e] 267 0

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