Göttgens F, Latour M, Heber U, Kamann S, Kremer K, Martens S, Dreizler S (2026)
Publication Type: Journal article
Publication year: 2026
Book Volume: 707
Article Number: A261
DOI: 10.1051/0004-6361/202558594
Binaries in the cores of globular clusters are known to prevent the gravitational collapse of the cluster, and simulations predict that the core of NGC 6397 contains a high number of white dwarfs (WDs), of which many are expected to be part of a binary system. In this work, we report the discovery of a compact binary system consisting of two WDs in the centre of the Galactic globular cluster NGC 6397. The system, known in the literature as NF1, was observed as part of a MUSE radial-velocity survey aiming at characterizing the binary population in the centre of NGC 6397. The spectral analysis of NF1 provides an effective temperature of 16 000 K and a surface gravity (log g) of 5.72 (cgs), which is consistent with the characteristics of an extremely low-mass He-core WD. This is further supported by the mass of 0.23 ± 0.03 M
APA:
Göttgens, F., Latour, M., Heber, U., Kamann, S., Kremer, K., Martens, S., & Dreizler, S. (2026). Discovery of a double white dwarf in the Galactic globular cluster NGC 6397. Astronomy & Astrophysics, 707. https://doi.org/10.1051/0004-6361/202558594
MLA:
Göttgens, Fabian, et al. "Discovery of a double white dwarf in the Galactic globular cluster NGC 6397." Astronomy & Astrophysics 707 (2026).
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