2020ApJ...904...24B


Query : 2020ApJ...904...24B

2020ApJ...904...24B - Astrophys. J., 904, 24-24 (2020/November-3)

Near-infrared opacity of late M dwarfs and hot Jupiters: the E3Π-X3Δ transition of TiO.

BERNATH P. and CAMERON W.D.

Abstract (from CDS):

The TiO E3Π-X3Δ transition is an important opacity source in the near-infrared spectra of late M dwarfs. The 0-0 band of the 48Ti16O E3Π-X3Δ electronic transition has been reanalyzed using a recently published set of high-resolution, high temperature absorption cross sections. The analysis has been extended to higher J values and an improved set of spectroscopic constants were determined. Calculated high-precision line lists for the 0-0 and 0-1 bands are provided with line strengths based on a previously measured experimental lifetime.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Laboratory astrophysics - Spectral line lists

Simbad objects: 4

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Number of rows : 4
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 * omi Cet Mi* 02 19 20.79210 -02 58 39.4956   7.63 6.53 5.03   M5-9IIIe+DA 1586 0
2 HD 15082b Pl 02 26 51.0582618096 +37 33 01.736482032           ~ 403 1
3 V* NP Aur S* 06 28 01.8021043320 +36 04 59.039512104           M5:S 21 0
4 V* VY CMa s*r 07 22 58.3261352189 -25 46 03.194390594 12.01 10.068 8.691 7.938   M5Iae 1169 0

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