The new FUor star HBC 722 - one year after the outburst

Details The new FUor star HBC 722 - one year after the outburst The new FUor star HBC 722 - one year after the outburst

2011-12-16

arxiv.org/abs/1112.3918v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Conference talk presented at the annual meeting of the Bulgarian Astronomical Union. Will be published in the Bulgarian Astron

Scientific paper

The first results from studies of the new FU Orionis star found in the field of NGC 7000 are presented in the paper. During the year passing from the registration of outburst at fourteen papers containing data from observations of this object have been published in the astronomical journals. These publications present photometric and spectral observations of HBC 722 ranging from the far infrared to X-ray wavelength region. HBC 722 is the first FU Orionis object, whose outburst was observed from its very beginning in all spectral ranges. We expect that the interest in this object will increase in the coming years and the results will help to explore the nature of young stars.

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