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The paper titled "Cremona problem in dimension 2" by W. Bartenwerfer presented a flawed attempt at proving the Jacobian Conjecture. Our aim is to provide a thorough analysis of the author's approach, highlighting the errors that were made…

代数几何 · 数学 2023-06-08 Szymon Brzostowski , Tadeusz Krasiński

This paper provides an overview of work, published since the opening of the archives of the Vatican Congregation for the Doctrine of the Faith at the end of the twentieth century, regarding the Vatican confronting evolution in the…

物理学史与哲学 · 物理学 2024-03-11 Christopher M. Graney

Early attempts to apply asteroseismology to study the Galaxy have already shown unexpected discrepancies for the mass distribution of stars between the Galactic models and the data; a result that is still unexplained. Here, we revisit the…

星系天体物理 · 物理学 2017-02-01 Sanjib Sharma , Dennis Stello , Daniel Huber , Joss Bland-Hawthorn , Timothy R. Bedding

The Kepler mission has been a success in both exoplanet search and stellar physics studies. Red giants have actually been quite a highlight in the Kepler scene. The Kepler long and almost continuous four-year observations allowed us to…

太阳与恒星天体物理 · 物理学 2017-11-08 Savita Mathur , Rafael A. Garcia , Daniel Huber , Clara Regulo , Dennis Stello , Paul G. Beck , Kenza Houmani , David Salabert

In this study we combine asteroseismic, spectroscopic and kinematic information to perform a detailed analysis of a sample of 16 stars from the Kepler field. Our selection focuses on stars that appear to contradict Galactic chemical…

太阳与恒星天体物理 · 物理学 2023-06-07 Arthur Alencastro Puls , Luca Casagrande , Stephanie Monty , David Yong , Fan Liu , Dennis Stello , Mikkel N. Lund

We present stellar properties (mass, age, radius, distances) of 57 stars from a seismic inference using full-length data sets from Kepler. These stars comprise active stars, planet-hosts, solar-analogs, and binary systems. We validate the…

We present a statistical analysis of the Kepler M dwarf planet hosts, with a particular focus on the fractional number of systems hosting multiple transiting planets. We manufacture synthetic planetary systems within a range of planet…

地球与行星天体物理 · 物理学 2017-03-08 Sarah Ballard , John Asher Johnson

The identity of Type Ia supernova progenitors remains a mystery, with various lines of evidence pointing towards either accretion from a non-degenerate companion, or the rapid merger of two degenerate stars leading to the thermonuclear…

太阳与恒星天体物理 · 物理学 2015-06-17 Wolfgang E. Kerzendorf , Michael Childress , Julia Scharwaechter , Tuan Do , Brian P. Schmidt

A number of Kepler planet pairs lie just wide of first-order mean motion resonances (MMRs). Tides have been frequently proposed to explain these pileups, but it is still an ongoing discussion. We contribute to this discussion by calculating…

地球与行星天体物理 · 物理学 2015-09-30 Ari Silburt , Hanno Rein

We describe a program to prove the Kepler conjecture on sphere packings. We then carry out the first step of this program. Each packing determines a decomposition of space into Delaunay simplices, which are grouped together into finite…

度量几何 · 数学 2007-05-23 Thomas C. Hales

October 2004 marks the 400th anniversary of the sighting of SN 1604, now marked by the presence of an expanding nebulosity known as Kepler's supernova remnant. Of the small number of remnants of historical supernovae, Kepler's remnant…

天体物理学 · 物理学 2007-05-23 W. P. Blair

It is now well established that Kepler's supernova remnant is the result of a Type Ia explosion. With an age of 407 years, and an angular diameter of ~ 4', Kepler is estimated to be between 3.0 and 7.0 kpc distant. Unlike other Galactic…

高能天体物理现象 · 物理学 2015-06-05 Daniel J. Patnaude , Carles Badenes , Sangwook Park , J. Martin Laming

Of the more than 150000 targets followed by the Kepler Mission, about 10% were selected as red giants. Due to their high scientific value, in particular for Galaxy population studies and stellar structure and evolution, their Kepler light…

太阳与恒星天体物理 · 物理学 2015-06-12 D. Stello , D. Huber , T. R. Bedding , O. Benomar , L. Bildsten , Y. P. Elsworth , R. L. Gilliland , B. Mosser , B. Paxton , T. R. White

Stars with hot Jupiters have obliquities ranging from 0-180 degrees, but relatively little is known about the obliquities of stars with smaller planets. Using data from the California-Kepler Survey, we investigate the obliquities of stars…

When low- and intermediate-mass stars evolve off the main sequence, they expand and cool into the red giant stages of evolution, which include those associated with shell H burning (the red giant branch), core He burning (the red clump),…

Hot Jupiters may have formed in situ, or been delivered to their observed short periods through one of two categories of migration mechanisms: disk migration or high-eccentricity migration. If hot Jupiters were delivered by…

地球与行星天体物理 · 物理学 2023-02-08 Jonathan M. Jackson , Rebekah I. Dawson , Billy Quarles , Jiayin Dong

We provide an overview of stellar variability in the first quarter of data from the Kepler mission. The intent of this paper is to examine the entire sample of over 150,000 target stars for periodic behavior in their lightcurves, and relate…

Recent data from the Kepler mission has revealed the occurrence of superflares in sun-like stars which exceed by far any observed solar flares in release of energy. A natural idea is that the dynamo mechanism in superflaring stars differs…

太阳与恒星天体物理 · 物理学 2018-03-14 M. M. Katsova , L. L. Kitchatinov , M. A. Livshits , D. L. Moss , D. D. Sokoloff , I. G. Usoskin

The Kepler mission and its successor K2 have brought forth a cascade of transiting planets. Many of these planetary systems exhibit multiple members, but a large fraction possess only a single transiting example. This overabundance of…

地球与行星天体物理 · 物理学 2018-04-11 Christopher Spalding , Noah W. Marx , Konstantin Batygin

$\eta_{\oplus}$, the occurrence rate of rocky habitable zone exoplanets orbiting Sun-like stars, is of great interest to both the astronomical community and the general public. The Kepler space telescope has made it possible to estimate…