Strong Neon Emission in CSS081007:030559+054715: A Possible Oxygen/ Neon Nova

Details Strong Neon Emission in CSS081007:030559+054715: A Possible Oxygen/ Neon Nova Strong Neon Emission in CSS081007:030559+054715: A Possible Oxygen/ Neon Nova

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1835....1p&link_type=abstract

The Astronomer's Telegram, #1835

Astronomy and Astrophysics

Astronomy

8

Optical, Novae, Transients

Scientific paper

On 2008 October 30.4 we obtained low-resolution optical spectra (range 3350-4800 Angstroms) of the transient CSS081007:030559+054715 using the Boller & Chivens CCD Spectrograph on the 1.3m McGraw-Hill telescope at MDM Observatory. The most striking feature in this spectral region is very strong, double-peaked [Ne V] at 3426 Angstroms. The two peaks are offset by -1700 and 1100 km/s with respect to the rest wavelength.

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