A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

Kavli Affiliate: Mark Vogelsberger | Summary:Precession is a very common phenomenon for small-scale astronomical objects. However, the precession of galactic disks, occurring on a scale larger than kilo-parsec, has barely been studied in the literature. Quantifying this precession in observations remains challenging due to the lack of high-resolution dynamical data. Cosmological simulations, where gravitational interactions […]


Continue.. A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

Kavli Affiliate: Mark Vogelsberger | Summary:Precession is a very common phenomenon for small-scale astronomical objects. However, the precession of galactic disks, occurring on a scale larger than kilo-parsec, has barely been studied in the literature. Quantifying this precession in observations remains challenging due to the lack of high-resolution dynamical data. Cosmological simulations, where gravitational interactions […]


Continue.. A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

Kavli Affiliate: Mark Vogelsberger | Summary:In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the Laser Interferometer Space Antenna (LISA) is to constrain the origin and growth of MBHs through their merger rates and mass […]


Continue.. The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

Fast radio burst dispersion is an unbiased tracer of matter on large scales

Kavli Affiliate: Kiyoshi Masui | Summary:The dispersion of fast radio bursts (FRBs) measures the column density of free electrons, tracing the diffuse ionized gas that contains more than $90%$ of all baryons. On linear scales the FRB dispersion field is an approximately unbiased tracer of the matter distribution, an idea long assumed in the FRB […]


Continue.. Fast radio burst dispersion is an unbiased tracer of matter on large scales

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation

Kavli Affiliate: Mark Vogelsberger | Summary:The origin and structure of the hot ($Tgtrsim10^6$ K) gaseous halo around Milky Way (MW)-mass galaxies provide a critical test for galaxy formation models. We perform a comprehensive comparison for a sample of MW analogues from the TNG50 cosmological simulation by generating synthetic soft X-ray emission and O VII/O VIII […]


Continue.. Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation

Kavli Affiliate: Mark Vogelsberger | Summary:The origin and structure of the hot ($Tgtrsim10^6$K) gaseous halo around Milky Way (MW)-mass galaxies provide a critical test for galaxy formation models. We perform a comprehensive comparison for a sample of MW analogues from the TNG50 cosmological simulation by generating synthetic soft X-ray emission and O VII/O VIII absorption […]


Continue.. Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation

Uncovering the Rapidly Evolving Orbits of the Dynamic TOI-201 System

Kavli Affiliate: Avi Shporer | Summary:Studying planetary interactions in exoplanet systems informs theories of planet formation and evolution, providing essential context for understanding our own solar system. We combine spectroscopy, transit photometry, transit timing variations, and astrometry to characterize the TOI-201 system. The co-transiting system consists of a super-Earth, warm Jupiter, and massive companion at […]


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Direct Imaging Constraints on Binary Planets and Exomoons around Epsilon Indi A b

Kavli Affiliate: Andrew Vanderburg | Summary:Epsilon Indi A b is a directly imaged $sim6 M_rm Jup$ exoplanet orbiting a nearby (3.6 pc) K-dwarf at $sim 30$ AU. We analyze archival JWST/MIRI 15 $μ$m coronagraphic imaging of this planet to search for directly imaged satellites orbiting Eps Ind A b. Within the planet’s Hill sphere (radius […]


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Unraveling Chemical Enrichment in Extreme Emission-Line Galaxies: A Multi-Element Bayesian View of Bursty Star Formation and Galaxy Evolution in DESI

Kavli Affiliate: Mark Vogelsberger | Summary:Extreme emission-line galaxies (EELGs) probe chemical enrichment in low-mass, bursty systems where star formation, feedback, and gas accretion are poorly constrained. Using DESI DR1, we select 23 nearby EELGs with detections of 19 ionic species (S/N $geq$ 4), stellar masses $ M_* geq 10^7 M_odot$, and extreme H$α$ and [O […]


Continue.. Unraveling Chemical Enrichment in Extreme Emission-Line Galaxies: A Multi-Element Bayesian View of Bursty Star Formation and Galaxy Evolution in DESI

Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode

Kavli Affiliate: Saul Rappaport | Summary:Aims. We are attempting to better understand how stellar pulsations in close binary systems are affected, and possibly induced, by tidal, Coriolis, and centrifugal forces. Methods. We analyzed TESS data for some 50,000 potential eclipsing binaries selected by machine learning algorithms in order to search for pulsation multiplets split by […]


Continue.. Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode