Near infrared studies of the massive X-ray binary 2S 0114+65

Details Near infrared studies of the massive X-ray binary 2S 0114+65 Near infrared studies of the massive X-ray binary 2S 0114+65

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38.2777a&link_type=abstract

Advances in Space Research, Volume 38, Issue 12, p. 2777-2778.

Computer Science

Scientific paper

We present near-infrared spectroscopy of the massive X-ray binary 2S 0114+650. These observations covering the spectral range 1.08 2.35 μm span the region where Paschen and Brackett series recombination lines of hydrogen are expected to be seen, namely, Paβ , Brγ and Br 10 17 lines. The absence of any of these lines in emission supports earlier inferences that the optical component in 2S 0114+650 is unlikely to be a Be star but rather a B type supergiant. Near-IR photometry gives J = 8.78, H = 8.53 and K = 7.96; these values show marginal variations from earlier reported measurements.

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