High Amplitude Variability in a Binary Candidate in the Orion Nebula Cluster

Details High Amplitude Variability in a Binary Candidate in the Orion Nebula Cluster High Amplitude Variability in a Binary Candidate in the Orion Nebula Cluster

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confq..27m&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 27-27"

Computer Science

Scientific paper

Using archive images obtained with HST/WFPC2 of the Orion Nebula Cluster, we have identified high amplitude photometric variability in a visual binary. The measured flux in broad-band filters in one of the components changes by over 3 magnitudes. The narrow-band filter magnitudes indicate that both components of the binary have H-alpha emission. Follow-up near-infrared spectroscopy shows an intriguing and variable spectrum.

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