Compass Reading student worksheet
... Draw a line toward the sun. Check what time it is – in this example it’s 4 PM Draw a line on the ground toward the sun. This line represents an hour hand. Now draw a line on the ground to where the 12 should be. Halfway between these two lines will point south. ...
... Draw a line toward the sun. Check what time it is – in this example it’s 4 PM Draw a line on the ground toward the sun. This line represents an hour hand. Now draw a line on the ground to where the 12 should be. Halfway between these two lines will point south. ...
Dynamics of Stars and Black Holes in Dense Stellar Systems:
... kinetic energy per unit mass (= Em, where Em is the mean energy per unit mass of the cluster) ...
... kinetic energy per unit mass (= Em, where Em is the mean energy per unit mass of the cluster) ...
A self-consistent empirical model atmosphere, abundance and
... non-solar, inhomogeneous chemistry and the atmospheric structure of CP stars. Similar to previous empirical stratification studies, we use high-quality spectroscopic observations to obtain the average chemical composition, vertical distribution of some of the most important elements, and place const ...
... non-solar, inhomogeneous chemistry and the atmospheric structure of CP stars. Similar to previous empirical stratification studies, we use high-quality spectroscopic observations to obtain the average chemical composition, vertical distribution of some of the most important elements, and place const ...
MK09_Presentation
... produced for X 3 Σ− state vibration-rotation transitions, up to v=6. • Line lists also produced for OH up to v=13. • Transformation equation doesn’t work as expected for OH, but intensities are an improvement compared to what’s currently available in HITRAN. • The combination of experimental and the ...
... produced for X 3 Σ− state vibration-rotation transitions, up to v=6. • Line lists also produced for OH up to v=13. • Transformation equation doesn’t work as expected for OH, but intensities are an improvement compared to what’s currently available in HITRAN. • The combination of experimental and the ...
PPT
... • The solution should pass through all three critical points. • The twist of magnetic field is proportional to distance, i.e., in far region, toroidal (azimuthal) magnetic field is dominant. ...
... • The solution should pass through all three critical points. • The twist of magnetic field is proportional to distance, i.e., in far region, toroidal (azimuthal) magnetic field is dominant. ...
How astronomers measure brightness and colours – the magnitude
... some commonly used filters is shown in figure 1. In general, filters used in various instruments are not exactly the same. This means that in order to compare the magnitudes of different measurements it is necessary to correct the magnitudes to the same filter system. The process of transforming the ...
... some commonly used filters is shown in figure 1. In general, filters used in various instruments are not exactly the same. This means that in order to compare the magnitudes of different measurements it is necessary to correct the magnitudes to the same filter system. The process of transforming the ...
Chapter 44 Problems
... As part of his discovery of the neutron in 1932, James Chadwick determined the mass of the newly identified particle by firing a beam of fast neutrons, all having the same speed, at two different targets and measuring the maximum recoil speeds of the target nuclei. The maximum speeds arise when an e ...
... As part of his discovery of the neutron in 1932, James Chadwick determined the mass of the newly identified particle by firing a beam of fast neutrons, all having the same speed, at two different targets and measuring the maximum recoil speeds of the target nuclei. The maximum speeds arise when an e ...
SRMP Solar System Curriculum - American Museum of Natural History
... Hand out a Moons of Jupiter sheet to all students along with colored pencils or markers. Explain that this is a simulation of Galileo’s data. (In fact, this is an idealized simulation, in that the data are given every 12 hours exactly, and there are no “cloudy” days where observations could not be m ...
... Hand out a Moons of Jupiter sheet to all students along with colored pencils or markers. Explain that this is a simulation of Galileo’s data. (In fact, this is an idealized simulation, in that the data are given every 12 hours exactly, and there are no “cloudy” days where observations could not be m ...
Two extremely luminous WN stars in the Galactic center with
... 2001; Simpson et al. 2007) surveys of the GC reveal a complex structure of the ionized gas with many small-scale compact sources of thermal emission. In this paper we investigate the emission from such nebulae around our program stars. ...
... 2001; Simpson et al. 2007) surveys of the GC reveal a complex structure of the ionized gas with many small-scale compact sources of thermal emission. In this paper we investigate the emission from such nebulae around our program stars. ...
Role of column density in the formation of stars
... For disc galaxies, the model assumes that a galaxy acquires most of its mass in a time that is short compared with the time required for the gas to turn into stars, and that the dark matter quickly settles into an isothermal sphere and the gas into a disc with the same radial mass distribution. Alth ...
... For disc galaxies, the model assumes that a galaxy acquires most of its mass in a time that is short compared with the time required for the gas to turn into stars, and that the dark matter quickly settles into an isothermal sphere and the gas into a disc with the same radial mass distribution. Alth ...
The fine-scale structure of dark matter halos
... Df / Dt = 0 only a 3-D subspace is occupied at all times. Nonlinear evolution leads to multi-stream structure and caustics ...
... Df / Dt = 0 only a 3-D subspace is occupied at all times. Nonlinear evolution leads to multi-stream structure and caustics ...
transparencies - Rencontres de Blois
... But with MOND (or modification of gravity) this is expected. ...
... But with MOND (or modification of gravity) this is expected. ...
High-mass stars in the Galactic center Quintuplet cluster
... in the Near-Infrared (SINFONI) to observe the central parts of the Quintuplet cluster in 22 fields of 8 × 8 arcsec field of view, see Fig. 1 with a background composite HST image (HST program 7364, PI D. Figer, NICMOS F110W, F160W, and F205W). A spectral catalog of the point sources with 160 flux-ca ...
... in the Near-Infrared (SINFONI) to observe the central parts of the Quintuplet cluster in 22 fields of 8 × 8 arcsec field of view, see Fig. 1 with a background composite HST image (HST program 7364, PI D. Figer, NICMOS F110W, F160W, and F205W). A spectral catalog of the point sources with 160 flux-ca ...
The Chandra Orion Ultradeep Project Eric Feigelson
... Even these weak COUP flares are ~10x stronger than the most powerful flares from the contemporary Sun. ...
... Even these weak COUP flares are ~10x stronger than the most powerful flares from the contemporary Sun. ...
Gamma-ray absorption and pair echos at very high
... the γγ opacity [6], [7]. On the other hand, UV radiation with ϵ < ϵLE have much longer mean free paths in the IGM, and the concept of a nearly uniform background may still be appropriate for this regime, which is also the most relevant for γγ absorption. Note in particular the band ϵ = 10.2 − 13.6 e ...
... the γγ opacity [6], [7]. On the other hand, UV radiation with ϵ < ϵLE have much longer mean free paths in the IGM, and the concept of a nearly uniform background may still be appropriate for this regime, which is also the most relevant for γγ absorption. Note in particular the band ϵ = 10.2 − 13.6 e ...
Self-similar evolution of wind-blown bubbles with mass
... expected to be aligned; thus, the assumption of unsaturated conduction with a T 5/2 temperature dependence of ρ̇, the mass evaporation rate per unit volume, should be reasonable throughout most of the mass-loading region if mass-loading is significant. We also assume that the clumps are stationary w ...
... expected to be aligned; thus, the assumption of unsaturated conduction with a T 5/2 temperature dependence of ρ̇, the mass evaporation rate per unit volume, should be reasonable throughout most of the mass-loading region if mass-loading is significant. We also assume that the clumps are stationary w ...
Grade 8 Writing a script for stories
... aluminium, silicon, phosphorus, sulphur, potassium, and iron. This is also true of the universe as a whole: Most of the universe is hydrogen, with some helium, and the remainder of the elements occur only in trace concentrations. So other stars are very similar in composition to our star, the sun ...
... aluminium, silicon, phosphorus, sulphur, potassium, and iron. This is also true of the universe as a whole: Most of the universe is hydrogen, with some helium, and the remainder of the elements occur only in trace concentrations. So other stars are very similar in composition to our star, the sun ...