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I review the results of recent cosmological simulations of galaxy formation that highlight the importance of satellite accretion in the formation of galactic disks. Tidal debris of disrupted satellites may contribute to the disk component…

Astrophysics · Physics 2016-01-27 Julio F. Navarro

Observations show that individual protoplanetary disk lifetimes vary from \mbox{$<$ 1 Myr} to $\gg$ 20 Myr. The disk lifetime distribution is currently unknown. For the example of a Gaussian distribution of the disk lifetime, I suggest a…

Astrophysics of Galaxies · Physics 2022-10-24 S. Pfalzner

Traditional Aboriginal Australian cultures include a significant astronomical component, perpetuated through oral tradition and ceremony. This knowledge has practical navigational and calendrical functions, and sometimes extends to a deep…

History and Philosophy of Physics · Physics 2010-09-27 Ray P. Norris , Duane W. Hamacher

The Maya were known for their astronomical proficiency. This is demonstrated in the Mayan codices where ritual practices were related to astronomical events/predictions. Whereas Mayan mathematics were based on a vigesimal system, they used…

History and Overview · Mathematics 2015-12-23 Thomas Chanier

We associate to any dynamical system with finitely many periodic orbits of each length a collection of possible time-changes of the sequence of periodic point counts that preserve the property of counting periodic points. Intersecting over…

Dynamical Systems · Mathematics 2020-11-30 Sawian Jaidee , Patrick Moss , Tom Ward

Sundial is the ancient or classic timekeeper device, especially prior to the invention of mechanical clock. In the classical Islamic civilization, the daily movement of the Sun becomes main indicator of praying time, which can be deduced…

Popular Physics · Physics 2013-12-11 Rhorom Priyatikanto

A variety of processes play a role in the evolution of protostellar disks. Here I focus on the uncertain issue of magnetic field-disk coupling and its implications for magnetically-driven turbulence and disk-driven winds. At present it is…

Astrophysics · Physics 2007-05-23 Mark Wardle

It is often assumed that a warped galaxy can be modeled by a set of rings. This paper verifies numerically the validity of this assumption by the study of periodic orbits populating a heavy self-gravitating warped disk. The phase space…

Astrophysics · Physics 2009-11-06 Y. Revaz , D. Pfenniger

Protoplanetary disks are quasi-steady structures whose evolution and dispersal determine the environment for planet formation. I review the theory of protoplanetary disk evolution and its connection to observations. Substantial progress has…

Solar and Stellar Astrophysics · Physics 2011-08-25 Philip J. Armitage

We review some of the interesting consequences that tilts, warps, and eccentricities can introduce into the dynamics, thermodynamics, and observational appearance of accreting systems, with an emphasis on disks around black holes and…

High Energy Astrophysical Phenomena · Physics 2026-03-04 P. Chris Fragile , Adam Ingram , Gibwa Musoke , Gordon I. Ogilvie

Astronomical observations and isotopic measurements of meteorites suggest that substructures are common in protoplanetary disks and may even have existed in the solar nebula. Here, we conduct paleomagnetic measurements of chondrules in CO…

It seems that the ancient Roman towns were oriented with the sunrise. Here I propose a discussion on the orientation of Torino, the Julia Augusta Taurinorum, which has the ancient Roman structure perfectly preserved. According to this…

Popular Physics · Physics 2012-08-10 Amelia Carolina Sparavigna

Protoplanetary disks are known to posses a stunning variety of substructure in the distribution of their mm~sized grains, predominantly seen as rings and gaps (Andrews et al. 2018), which are frequently interpreted as due to the shepherding…

Earth and Planetary Astrophysics · Physics 2019-10-17 Richard Teague , Jaehan Bae , Edwin Bergin

The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities. Thus, to fully understand galactic disks, we must study their stellar kinematics as well as their morphologies. Observational techniques have now…

Astrophysics · Physics 2007-05-23 Michael R. Merrifield , Konrad Kuijken

We studied near-infrared disk fractions of six young clusters in the low-metallicity environments with [O/H$] \sim -0.7$ using deep $JHK$ images with Subaru 8.2\,m telescope. We found that disk fraction of the low-metallicity clusters…

Solar and Stellar Astrophysics · Physics 2015-05-20 Chikako Yasui , Naoto Kobayashi , Alan T. Tokunaga , Masao Saito , Chihiro Tokoku

We present the results of our studies on accretion disks in the proximity of astrophysical black holes. These disks can be of varying degrees of opacity, geometrical shapes, sizes, and volumes. The central compact object is a Schwarzschild…

High Energy Astrophysical Phenomena · Physics 2023-02-27 Leela Elpida Koutsantoniou

Given their proximity and age differences, nearby groups of young stars are valuable laboratories for investigations of disk evolution and diversity. The estimated 10-Myr age of groups like the TW Hydrae Association provides a strong…

Astrophysics · Physics 2007-05-23 Ray Jayawardhana

The digitization of historical astronomical plates is essential for preserving century-long observational data. This work presents the development and application of the specialized digitizers at the Shanghai Astronomical Observatory…

Instrumentation and Methods for Astrophysics · Physics 2025-10-13 Yong Yu , Meiting Yang , Zhengjun Shang , Liangliang Wang , Jing Yang , Zhenghong Tang , Jianhai Zhao , Massinissa Hadjara

The Long Now Foundation is building a mechanical clock that is designed to keep time for the next 10,000 years. The clock maintains its long-term accuracy by synchronizing to the Sun. The 10,000-Year Clock keeps track of five different…

Instrumentation and Methods for Astrophysics · Physics 2011-12-14 Danny Hillis , Rob Seaman , Steve Allen , Jon Giorgini

In binary systems with a strongly misaligned disk, the central binary stars can travel a significant vertical distance above and below the disk's orbital plane. This can cause large changes in illumination of the disk over the course of the…

Earth and Planetary Astrophysics · Physics 2026-01-14 Ian Rabago , Giuseppe Lodato , Stefano Facchini , Zhaohuan Zhu
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