We report on the identification of the optical counterpart to Star1, the exotic object serendipitously discovered by Deutsch et al. in the core of the Galactic globular cluster NGC 6624. Star1 has been classified by Deutsch et al. as either a quiescent Cataclysmic Variable or a low-mass X-ray binary. Deutsch et al. proposedStarA as possible optical counterpart to this object. We used high-resolution images obtained with the Hubble Space Telescope to perform a variability analysis of the stars close to the nominal position of Star1. While no variability was detected for StarA, we found another star, here named COM_Star1, showing a clear sinusoidal light modulation with amplitude ∆m F435W ∼ 0.7mag and orbital period of P orb ∼ 98min. The shape of the light curve is likely caused by strong irradiation by the primary heating one hemisphere of the companion, thus suggesting a quite hot primary.

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Individual, social and situational factors might play an important role on the experience of anxiety during musical performances. The present research focused on the relationship between self-representations, including musical self, and performance anxiety among a sample of Italian professional and amateur musicians (N = 100; age, M = 23.40, 50% females). We predicted that higher self-discrepancies (actual vs. future self) would be associated with higher performance anxiety in a musical setting (vs. a non musical one), via musical self, and only in professional musicians. The results confirmed our hypothesis. Higher discrepancies between actual and future self-representations were positively associated with higher performance anxiety levels via the musical self only in participants who play instruments at a professional level. Furthermore, musical self influenced performance anxiety levels in a music related setting (i.e., a concert) but not in a non musical one (i.e., an exam).

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