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2026RNAAS..10....2R - Research Notes of the AAS, 10, 2 (2026/January-0)
Infrared Spectroscopy of the Nova V5115 Sagittarii during Its Fe II Phase.
RUDY R.J., RUSSELL R.W. and LYNCH D.K.
Abstract (from CDS):
V5115 Sagittarii was a very fast nova (t2 = 7 days) from a massive white dwarf (1.2 M⊙). Our 0.8-5.0 μm spectrum from 19 days after discovery shows numerous Fe II lines and weak, just emerging He I emission and falls clearly within the Fe II-type nova classification. At this epoch, the nova had sufficient excitation that N I features were plentiful but Na I emission was absent and only the brightest C I features were detectable.
Abstract Copyright: © 2026. The Author(s). Published by the American Astronomical Society.
Journal keyword(s): Classical novae
Simbad objects: 3
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