Evidence of infalling matter in Mira

Details Evidence of infalling matter in Mira Evidence of infalling matter in Mira

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...133l...1f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 133, no. 1, April 1984, p. L1-L3.

Astronomy and Astrophysics

Astrophysics

13

Line Shape, Mira Variables, Stellar Mass Accretion, Stellar Spectra, Variable Stars, Cygnus Constellation, High Resolution, Shock Wave Propagation, Signal To Noise Ratios, Spectral Resolution, Supersonic Speed

Scientific paper

The authors report the first spectroscopic observation of Mira at high
resolution (100 mÅ) around 1 micron. It reveals inverse P Cygni
profiles of neutral titanium. These are interpreted in terms of direct
evidence of infalling matter, with supersonic velocities.

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