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Sökning: id:"swepub:oai:research.chalmers.se:1ac2fdd5-76ea-40fe-b427-8d802aece103" > On the detection of...

On the detection of CO and mass-loss of bulge OH/IR stars

Blommaert, Jadl (författare)
Vrije Universiteit Brüssel (VUB),Vrije Universiteit Brussel (VUB)
Groenewegen, M. A. T. (författare)
Royal Observatory of Belgium
Justtanont, Kay, 1965 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
visa fler...
Decin, L. (författare)
Katholieke Universiteit Leuven
visa färre...
 (creator_code:org_t)
2018-06-25
2018
Engelska.
Ingår i: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 479:3, s. 3545-3562
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • We report on the successful search forCO(2-1) and (3-2) emission associated with OH/IR stars in the Galactic bulge. We observed a sample of eight extremely red asymptotic giant branch stars with the Atacama Pathfinder EXperiment telescope and detected seven. The sources were selected at a sufficiently high galactic latitude to avoid interference by interstellar CO, which hampered previous studies of inner galaxy stars. To study the nature of our sample and the mass-loss, we constructed the spectral energy distribution (SEDs) from photometric data and Spitzer IRS spectroscopy. In a first step, we apply radiative transfer modelling to fit the SEDs and obtain luminosities and dust mass-loss rates (MLRs). Through dynamical modelling, we then retrieve the total MLR and the gas-to-dust ratios. We derived variability periods of our stars. The luminosities range between approximately 4000 and 5500 L⊙and periods are shorter than 700 d. The total MLR ranges between 10-5and 10-4M⊙yr-1. Comparison with evolutionary models shows that the progenitor mass ≈ 1.5 M⊙, similar to the bulge Miras of intermediate age (3 Gyr). The gas-to-dust ratios are between 100 and 400 and are similar to what is found for OH/IR stars in the galactic disc. One star, IRAS 17347-2319, has a very short period of approximately 300 d that may be decreasing further. It may belong to a class of Mira variables with a sudden change in period as observed in some Galactic objects. It would be the first example of an OH/IR star in this class and deserves further follow-up observations.

Ämnesord

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Matematik -- Sannolikhetsteori och statistik (hsv//swe)
NATURAL SCIENCES  -- Mathematics -- Probability Theory and Statistics (hsv//eng)

Nyckelord

Stars: mass-loss
Stars: AGB and post-AGB
Radio lines: stars
Circumstellar matter
Galaxy: bulge

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