'Burning' presentation slideshows

Lecture 15 Explosive Nucleosynthesis and the r-Process

Lecture 15 Explosive Nucleosynthesis and the r-Process. As the shock wave passes through the star, matter is briefly heated to temperatures far above what it would have experienced in hydrostatic equilibrium. This material expands, then cools nearly adiabatically

836 views • 73 slides

Lecture 11 Neutrino Losses and Advanced Stages of Stellar Evolution - I

Lecture 11 Neutrino Losses and Advanced Stages of Stellar Evolution - I. The late stages (> helium burning) of evolution in massive stars are characterized by huge luminosities, carried away predominantly by neutrinos, and consequently by short time scales.

838 views • 69 slides

Syphilis

Syphilis. -Spiral shaped spirochete (Treponema pallidum) -gram negative, but does not have lipopolysaccharide (LPS) -helical, thin (0.1 to 0.2 um), and long -flagella are inserted into the periplasm and give it motility -sensitive to drying, chemicals, and heat (as low as 42 degrees celsius).

1.14k views • 62 slides

MASSIVE STARS: PRESUPERNOVA EVOLUTION, EXPLOSION AND NUCLEOSYNTHESIS

929 views • 59 slides

594 views • 38 slides

Alessandro Chieffi

527 views • 38 slides

Emission Inventory Sources

Emission Inventory Sources. Goals. Indicators . Strategies. Acronym Definitions. AQ: Air Quality PM 10 : Particulate Matter with a diameter of 10 microns (1*10e -6 metres) or less. PM 2.5 : Particulate Matter with a diameter of 2.5 microns (1*10e -6 metres) or less.

443 views • 31 slides

SURVIVOR:

SURVIVOR: . How to Keep Your Torch Burning !. SURVIVOR: How to Keep Your Torch Burning!. Presented by: Barbara Donati Joan Kelly Rafferty, OTR/L. SURVIVOR: How to Keep Your Torch Burning!. Learning Objectives The participant will:

500 views • 28 slides

Fahrenheit 451

Fahrenheit 451. Ray Bradbury. Conflicts. An external conflict between Montag, who rejects book burning, and the fire captain, who defends it

714 views • 22 slides

Positively Parliament

334 views • 21 slides

Lars Bildsten Kavli Institute for Theoretical Physics University of California Santa Barbara

Putting Helium Layers onto Massive White Dwarfs. Lars Bildsten Kavli Institute for Theoretical Physics University of California Santa Barbara.

358 views • 20 slides

Open Burning Logging Slash in Beetle Wood Harvesting Areas of British Columbia.

Open Burning Logging Slash in Beetle Wood Harvesting Areas of British Columbia. Meeting MOF and WLAP Requirements E. Plain, Air Quality Meteorologist Cariboo Region. Issue:.

288 views • 19 slides

On the Nature of the Thermal Pulses on the Asymptotic Giant Branch Alessandro Chieffi

334 views • 19 slides

Global Warming

Global Warming. BY SAIMA SOHAIL THE CITY SCHOOL DARAKHSHAN CAMPUS. What is global warming?. The changes in the surface air temperature, referred to as the global temperature, brought about by the enhanced greenhouse effect, which is induced by emissions of greenhouse gases into the air.

739 views • 16 slides

The s-process in massive stars

343 views • 16 slides

10. NUCLEAR PROCESSES IN THE LATE STAGES OF THE EVOLUTION OF MASSIVE STARS

}. Na 23 + p Ne 20 + a Mg 23 + n. 10. NUCLEAR PROCESSES IN THE LATE STAGES OF THE EVOLUTION OF MASSIVE STARS. 10.1 THE EFFECT OF MASS.

300 views • 15 slides

Town Meeting 2007 Article 31

Town Meeting 2007 Article 31. Statement of the Board of Health Town of Sudbury. Board of Health Vote. On March 8, 2007, the Board of Health voted to take NO POSITION on Article 31.

279 views • 14 slides

Dodging and Burning

Dodging and Burning. The art of adding or subtracting light from your print. Dodging subtracts light. Burning adds light. Gives the photographer more creative choices. Mapping your print. X=darken O=Lighten CS+=more contrast CS-=less contrast See also page 131 for another version.

250 views • 9 slides

English B1A

145 views • 6 slides

Unit 5: Democratic and Territorial Expansion (1824-1853)

444 views • 6 slides