SIMBAD references

2015ApJ...811...45S - Astrophys. J., 811, 45 (2015/September-3)

Infrared spectral properties of M giants.

SLOAN G.C., GOES C., RAMIREZ R.M., KRAEMER K.E. and ENGELKE C.W.

Abstract (from CDS):

We observed a sample of 20 M giants with the Infrared Spectrograph on the Spitzer Space Telescope. Most show absorption structure at 6.6-6.8 µm which we identify as water vapor, and in some cases, the absorption extends from 6.4 µm into the SiO band at 7.5 µm. Variable stars show stronger H2 O absorption. While the strength of the SiO fundamental at 8 µm increases monotonically from spectral class K0 to K5, the dependence on spectral class weakens in the M giants. As with previously studied samples, the M giants show considerable scatter in SiO band strength within a given spectral class. All of the stars in our sample also show OH band absorption, most noticeably in the 14-17 µm region. The OH bands behave much like the SiO bands, increasing in strength in the K giants but showing weaker dependence on spectral class in the M giants, and with considerable scatter. An examination of the photometric properties reveals that the color may be a better indicator of molecular band strength than the spectral class. The transformation from Tycho colors to Johnson color is double-valued, and neither nor color increases monotonically with spectral class in the M giants like they do in the K giants.

Abstract Copyright:

Journal keyword(s): infrared: stars - stars: AGB and post-AGB

VizieR on-line data: <Available at CDS (J/ApJ/811/45): table1.dat sp/*>

Status at CDS:  

Simbad objects: 58

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2020.04.08-15:14:35

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