2018ApJ...863..139T


Query : 2018ApJ...863..139T

2018ApJ...863..139T - Astrophys. J., 863, 139-139 (2018/August-3)

Is AlOH the astrochemical reservoir molecule of AlO?: insights from excited electronic states.

TRABELSI T. and FRANCISCO J.S.

Abstract (from CDS):

Very recently, the optical bands of the 2Σ+ - X2Σ+system of AlO have been identified in the red supergiant star VYCMa. In an effort to explain the origin of this transition, we used state-of-the-art quantum chemical calculations with proven high accuracy to compute the lowest singlet and triplet electronic states of the AlOH and HAlO isomers as well as their equilibrium geometry and electronic properties. Our calculated potential energy surfaces implicate the three singlet electronic states 21A', 31A', and 11A'' in the photodissociation of the [Al,O,H] system. Only AlO, H, Al, and OH products can occur through the photodissociation of [Al,O,H]; AlH and O are not allowed. For the photodissociation of AlOH, the AlO product can occur only in its excited states AlO(2Π) and AlO(2Σ+).

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): astrochemistry - supergiants - techniques: spectroscopic - ultraviolet: ISM

Simbad objects: 2

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Number of rows : 2
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 V* VY CMa s*r 07 22 58.3261352189 -25 46 03.194390594 12.01 10.068 8.691 7.938   M5Iae 1169 0
2 IRC +10216 C* 09 47 57.40632 +13 16 43.5648           C9,5e 2455 0

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