First Near Infrared Spectrum of V1118Ori

Details First Near Infrared Spectrum of V1118Ori First Near Infrared Spectrum of V1118Ori

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..619....1d&link_type=abstract

The Astronomer's Telegram, #619

Astronomy and Astrophysics

Astronomy

3

Infra-Red, Variables

Scientific paper

On (Sept. 11, 2005) the first near infrared (0.87 2.35 μm) spectrum of the EXOR variable V1118Ori was obtained in low resolution mode (R ~ 250), with the AZT24 telescope at Campo Imperatore (Italy). It presents strong hydrogen recombination lines of the Brackett and Paschen series, some ionic emission features possibly attributable to [FeII], and also emission in the overtone bands of CO (v = 2-0, v = 3-1).

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