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- ItemA low pre-infall mass for the Carina dwarf galaxy from disequilibrium modeling([London] : Nature Publishing Group UK, 2015) Ural, Uğur; Wilkinson, Mark I.; Read, Justin I.; Walker, Matthew G.Dark matter-only simulations of galaxy formation predict many more subhalos around a Milky Way-like galaxy than the number of observed satellites. Proposed solutions require the satellites to inhabit dark matter halos with masses 109–1010Msun at the time they fell into the Milky Way. Here we use a modelling approach, independent of cosmological simulations, to obtain a pre-infall mass of Msun for one of the Milky Way’s satellites: Carina. This determination of a low halo mass for Carina can be accommodated within the standard model only if galaxy formation becomes stochastic in halos below ∼1010Msun. Otherwise Carina, the eighth most luminous Milky Way dwarf, would be expected to inhabit a significantly more massive halo. The implication of this is that a population of ‘dark dwarfs’ should orbit the Milky Way: halos devoid of stars and yet more massive than many of their visible counterparts.
- ItemX-ray quasi-periodic eruptions from two previously quiescent galaxies(London [u.a.] : Nature Publ. Group, 2021) Arcodia, R.; Merloni, A.; Nandra, K.; Buchner, J.; Salvato, M.; Pasham, D.; Remillard, R.; Comparat, J.; Lamer, G.; Ponti, G.; Malyali, A.; Wolf, J.; Arzoumanian, Z.; Bogensberger, D.; Buckley, D.A.H.; Gendreau, K.; Gromadzki, M.; Kara, E.; Krumpe, M.; Markwardt, C.; Ramos-Ceja, M.E.; Rau, A.; Schramm, M.; Schwope, A.Quasi-periodic eruptions (QPEs) are very-high-amplitude bursts of X-ray radiation recurring every few hours and originating near the central supermassive black holes of galactic nuclei1,2. It is currently unknown what triggers these events, how long they last and how they are connected to the physical properties of the inner accretion flows. Previously, only two such sources were known, found either serendipitously or in archival data1,2, with emission lines in their optical spectra classifying their nuclei as hosting an actively accreting supermassive black hole3,4. Here we report observations of QPEs in two further galaxies, obtained with a blind and systematic search of half of the X-ray sky. The optical spectra of these galaxies show no signature of black hole activity, indicating that a pre-existing accretion flow that is typical of active galactic nuclei is not required to trigger these events. Indeed, the periods, amplitudes and profiles of the QPEs reported here are inconsistent with current models that invoke radiation-pressure-driven instabilities in the accretion disk5–9. Instead, QPEs might be driven by an orbiting compact object. Furthermore, their observed properties require the mass of the secondary object to be much smaller than that of the main body10, and future X-ray observations may constrain possible changes in their period owing to orbital evolution. This model could make QPEs a viable candidate for the electromagnetic counterparts of so-called extreme-mass-ratio inspirals11–13, with considerable implications for multi-messenger astrophysics and cosmology14,15.