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Articles 1 - 7 of 7

Full-Text Articles in Physical Sciences and Mathematics

X-Ray Emission From O Stars, David H. Cohen Dec 2007

X-Ray Emission From O Stars, David H. Cohen

Physics & Astronomy Faculty Works

Young O stars are strong, hard, and variable X-ray sources, properties which strongly affect their circumstellar and galactic environments. After ~1 Myr, these stars settle down to become steady sources of soft X-rays. I use high-resolution X-ray spectroscopy and MHD modeling to show that young O stars like theta-1 Ori C are well explained by the magnetically channeled wind shock scenario. After their magnetic fields dissipate, older O stars produce X-rays via shock heating in their unstable stellar winds. Here too I use X-ray spectroscopy and numerical modeling to confirm this scenario. In addition to elucidating the nature and cause …


X-Rays From Magnetically Channeled Winds Of Ob Stars, In 'Magnetic Massive Stars', David H. Cohen Dec 2007

X-Rays From Magnetically Channeled Winds Of Ob Stars, In 'Magnetic Massive Stars', David H. Cohen

Physics & Astronomy Faculty Works

OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong and hard X-ray emission via the Magnetically Channeled Wind Shock (MCWS) mechanism. In this brief paper, I describe four separate X-ray diagnostics of the MCWS mechanism in OB stars, with applications to the prototype young O star, theta-1 Ori C.


Far-Off-Resonant Ring Trap Near The Ends Of Optical Fibers, Frank Moscatelli, C. Sackett, S. Du, E. Oh Oct 2007

Far-Off-Resonant Ring Trap Near The Ends Of Optical Fibers, Frank Moscatelli, C. Sackett, S. Du, E. Oh

Physics & Astronomy Faculty Works

We propose that micrometer-sized atom traps can be created using the optical dipole force between the ends of two single-mode optical fibers carrying counterpropagating light beams of two different wavelengths from both fibers. The traps have a simple design that is feasible to implement with commercially available products. They can be used as a flexible “atom tweezer” to manipulate atoms in free space without the need for traditional focused laser beams. A particularly interesting feature is the formation of a static ring-shaped trap for properly chosen beam parameters. Furthermore, this ring can be split into two longitudinally adjacent rings. Microscopic …


Periodic Accretion From A Circumbinary Disk In The Young Binary Uz Tau E, Eric L.N. Jensen, Saurav Dhital , '06, K. G. Stassun, J. Patience, W. Herbst, F. M. Walter, M. Simon, G. Basri Jul 2007

Periodic Accretion From A Circumbinary Disk In The Young Binary Uz Tau E, Eric L.N. Jensen, Saurav Dhital , '06, K. G. Stassun, J. Patience, W. Herbst, F. M. Walter, M. Simon, G. Basri

Physics & Astronomy Faculty Works

Close pre-main-sequence binary stars are expected to clear central holes in their protoplanetary disks, but the extent to which material can flow from the circumbinary disk across the gap onto the individual circumstellar disks has been unclear. In binaries with eccentric orbits, periodic perturbation of the outer disk is predicted to induce mass flow across the gap, resulting in accretion that varies with the binary period. This accretion may manifest itself observationally as periodic changes in luminosity. Here we present a search for such periodic accretion in the pre-main-sequence spectroscopic binary UZ Tau E. We present BVRI photometry spanning 3 …


Winning Paths In N-By-Infinity Hex, Walter Stromquist Mar 2007

Winning Paths In N-By-Infinity Hex, Walter Stromquist

Mathematics & Statistics Faculty Works

In n x ∞ Hex the player whose task is to complete a finite path can win, but the other player can ensure that any winning path contains at least n + [n−2/4] cells.


A 2007 Model Curriculum For A Liberal Arts Degree In Computer Science, Liberal Arts Computer Science Consortium, Charles F. Kelemen Feb 2007

A 2007 Model Curriculum For A Liberal Arts Degree In Computer Science, Liberal Arts Computer Science Consortium, Charles F. Kelemen

Computer Science Faculty Works

No abstract provided.


Projectional Entropy In Higher Dimensional Shifts Of Finite Type, Aimee S. A. Johnson, S. Kass, K. M. Madden Jan 2007

Projectional Entropy In Higher Dimensional Shifts Of Finite Type, Aimee S. A. Johnson, S. Kass, K. M. Madden

Mathematics & Statistics Faculty Works

Any higher dimensional shift space (X, ℤᵈ) contains many lower dimensional shift spaces obtained by projection onto r-dimensional sublattices L of ℤᵈ where r < d. We show here that any projectional entropy is bounded below by the ℤᵈ entropy and, in the case of certain shifts of finite type satisfying a mixing condition, equality is achieved if and only if the shift of finite type is the infinite product of a lower dimensional projection.