Moozonian

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arxiv.org
arxiv.org › abs › 1202.6387v2
Dynamics of stars around spiral arms in an N-body/SPH simulated barred-spiral galaxy
We run N-body smoothed particle hydrodynamics (SPH) simulations of a Milky Way sized galaxy. The code takes into account hydrodynamics, self-gravity, star formation, supernova and stellar wind feedbac...
arxiv.org
arxiv.org › abs › 2111.01843v2
Visibility Properties of Spiral Sets
A spiral in $\mathbb{R}^{d+1}$ is defined as a set of the form $\left\{\sqrt[d+1]{n}\cdot\boldsymbol{u}_n\right\}_{n\ge 1},$ where $\left(\boldsymbol{u}_n\right)_{n\ge 1}$ is a spherical sequence. Suc...
www.reddit.com
reddit.com › r › bourb...ood_spiral_finished ›
Review #99: 13th Colony Maple Wood Spiral Finished Bourbon
Up next, we're taking a look at the 13th Colony Maple Wood Spiral Finish! This was a limited release from 13th Colony that dropped earlier this year that a lot of people, unsurprisingly, went crazy ov...
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arxiv.org
arxiv.org › abs › astro-ph › 0305472v1
An H-alpha survey aiming at the detection of extraplanar diffuse ionized gas in halos of edge-on spiral galaxies II. The H-alpha survey atlas and catalog
In this second paper on the investigation of extraplanar diffuse ionized gas in nearby edge-on spiral galaxies we present the actual results of the individual galaxies of our H-alpha imaging survey. A...
arxiv.org
arxiv.org › abs › astro-ph › 0310341v2
HCN Survey of Normal Spiral, IR-luminous and Ultraluminous Galaxies
We report systematic HCN J=1-0 (and CO) observations of a sample of 53 infrared (IR) and/or CO-bright and/or luminous galaxies, including seven ultraluminous infrared galaxies, nearly 20 luminous infr...
arxiv.org
arxiv.org › abs › 1011.3446v1
Accretion Discs with an Inner Spiral Density Wave
In Montgomery (2009a), we show that accretion discs in binary systems could retrogradely precess by tidal torques like the Moon and the Sun on a tilted, spinning, non-spherical Earth. In addition, we ...
news.ycombinator.com
news.ycombinator.com › item?id=47046624
Show HN: A hands-on protocol to stop the "Implementation Death Spiral"
Points: 3 | Comments: 5 | Author: apetchesi
arxiv.org
arxiv.org › abs › 2111.01821v1
ESO 137-002: a large spiral undergoing edge-on ram-pressure stripping with little star formation in the tail
Ram pressure stripping (RPS) is an important mechanism for galaxy evolution. In this work, we present results from HST and APEX observations of one RPS galaxy, ESO 137-002 in the closest rich cluster ...
arxiv.org
arxiv.org › abs › astro-ph › 0103374v1
A Catalog of OB Associations in the spiral galaxy NGC 300
We present results of a search for OB associations in NGC 300. Using an automatic and objective method (PLC technique) 117 objects were found. Statistical tests indicate that our sample is contaminate...
arxiv.org
arxiv.org › abs › 1008.4201v2
Cornu's spiral in the Fresnel regime studied using ultrasound: A phase study
A simple experimental technique for measuring the phase and amplitude of diffracting ultrasound wave [A. Hitachi and M. Takata, Am. J. Phys. 78, 678 (2010)] has been applied to diffracting objects wit...
www.reddit.com
reddit.com › r › recru..._is_worse_than_2008 ›
The current job market crisis is worse than 2008. It's not a cycle, it's a downward spiral.
I was in middle school when the 2008 recession went into full swing, and I remember those days quite distinctly despite not necessarily being old enough to comprehend the full scale of the disaster. U...
health.yahoo.com
health.yahoo.com › your-...-stop-123817834.html
Winter Hair Loss Is Real—Here’s How to Stop the Seasonal Shedding Spiral, According to Experts
Cold weather can disrupt your hair growth cycle. Here’s how to tell the difference between seasonal shedding and something more serious.
arxiv.org
arxiv.org › abs › astro-ph › 0702433v1
Nuclear Star Clusters (Nuclei) in Spiral Galaxies and Connection to Supermassive Black Holes
HST observations have revealed that compact sources exist at the centers of many, maybe even most, galaxies across the Hubble sequence. These sources are called "nuclei" or also "nuclear star clusters...
arxiv.org
arxiv.org › abs › patt-sol › 9709004v1
Kinematic Equations for Front Motion and Spiral-Wave Nucleation
We present a new set of kinematic equations for front motion in bistable media. The equations extend earlier kinematic approaches by coupling the front curvature with the order parameter associated wi...
www.slideshare.net
slideshare.net › sli...-of-viruses › 52683399
Structural symmetry of viruses | PPTX - SlideShare
Viruses exhibit different types of structural symmetry including helical, icosahedral, complex, and envelope symmetries. Helical viruses form tube-like capsids from repeating protein subunits in a spi...
arxiv.org
arxiv.org › abs › 1211.0188v1
Galactic rotation curves in conformal gravity
We review some recent work by Mannheim and O'Brien on the systematics of galactic rotation curves in the conformal gravity theory. In this work the conformal theory was applied to a comprehensive, hig...
arxiv.org
arxiv.org › abs › physics › 0603026v1
Elements, topology, and T-shirts
Consider the network of elements connected by adjacency in atomic number and periodic table column. If all elements except H-He are connected by identical springs and constrained to a z-spiral in 2D, ...
arxiv.org
arxiv.org › abs › astro-ph › 0407413v1
3D MHD Modeling of the Gaseous Structure of the Galaxy: Synthetic Observations
We generated synthetic observations from the four-arm model presented in Gomez & Cox (2004) for the Galactic ISM in the presence of a spiral gravitational perturbation. We found that velocity crowding...
arxiv.org
arxiv.org › abs › 2205.11144v2
A Radio Continuum Study of NGC 2082
We present radio continuum observations of NGC 2082 using ASKAP, ATCA and Parkes telescopes from 888 MHz to 9000 MHz. Some 20 arcsec from the centre of this nearby spiral galaxy, we discovered a brigh...