Narrow-band infrared photometry of the peculiar white dwarf LHS 1126

Details Narrow-band infrared photometry of the peculiar white dwarf LHS 1126 Narrow-band infrared photometry of the peculiar white dwarf LHS 1126

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...278l.111l&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 278, March 15, 1984, p. L111-L114.

Astronomy and Astrophysics

Astronomy

9

Astronomical Photometry, Infrared Astronomy, Infrared Photometry, Peculiar Stars, Stellar Spectra, White Dwarf Stars, Narrowband, Near Infrared Radiation, Ultraviolet Spectra

Scientific paper

New infrared observations from 1.25 to 2.50 microns at 5 percent resolution are discussed for the cool white dwarf LHS 1126. These reveal a strong, smooth absorption at 2.0-2.3 microns and strong, structured absorption near 1.6 microns. These absorptions are not readily interpretable as either molecular hydrogen or molecular carbon. Comparison is also made with other stars observed in the infrared, but the spectrum of LHS 1126 is unique.

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