Does the HR 6819 triple system contain a dormant black hole? Not necessarily

ABSTRACT A recent paper by Rivinius et al. proposed that HR 6819 is a triple system, with a distant Be star and a binary of 40-d orbit, composed of a B3 III giant and a dormant black hole (BH). We suggest that the evidence for this model is not conclusive. In an alternative model, the companion of t...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society. Letters 2020-10, Vol.498 (1), p.L58-L60
Hauptverfasser: Mazeh, Tsevi, Faigler, Simchon
Format: Artikel
Sprache:eng
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Zusammenfassung:ABSTRACT A recent paper by Rivinius et al. proposed that HR 6819 is a triple system, with a distant Be star and a binary of 40-d orbit, composed of a B3 III giant and a dormant black hole (BH). We suggest that the evidence for this model is not conclusive. In an alternative model, the companion of the giant is by itself a short-period binary in, say, a ∼4-d orbit, consisting, for example, of two A0 stars. Each of the two A0 stars should contribute ${\sim}4{{\ \rm per cent}}$ of the total brightness of the system in the V band, and their spectral lines are moving due to their assumed orbital motion with an unknown period. Therefore, only a careful analysis of the observed spectra can exclude such a model. Before such an analysis is presented and upper limits for the depths of the hypothetical A0 star absorption lines are derived, the model of a hidden close pair is more probable than the BH model.
ISSN:1745-3925
1745-3933
DOI:10.1093/mnrasl/slaa124