Spectroscopic confirmation of HBC 722 as a new FU Orionis star in NGC 7000

Details Spectroscopic confirmation of HBC 722 as a new FU Orionis star in NGC 7000 Spectroscopic confirmation of HBC 722 as a new FU Orionis star in NGC 7000

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2808....1m&link_type=abstract

The Astronomer's Telegram, #2808

Astronomy and Astrophysics

Astronomy

4

Optical, Variables

Scientific paper

The photometric discovery of an outburst from HBC 722, a faint emission line object in the region of NGC 7000/IC 5070, has been recently reported in ATel #2801, where a nature similar to FU Orionis pre-Main sequence objects has been proposed. We have obtained a low resolution spectrum of HBC 722 on Aug. 21.9 UT with the 0.6m telescope of the Schiaparelli Observatory in Varese, equipped with a multi-mode grating spectrograph.

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