where can i find research information on the energy distribution from stars?
414661
http://xxx.lanl.gov/\nit is trusted site for any physical, astrophysical, cosmological issues.\nRegards
582743
Maybe the program 'Cartes du Ciel' can help you. You can download it for free in English at:\n\nhttp://www.stargazing.net/astropc/index.html
1145113
This should help you:  http://www.le.ac.uk/physics/faulkes/web/stars/o_st_overview.html
489152
They are made of hydrogen.  There's so much gravity at the core of a star that it compresses protons and electrons from other hydrogen atoms and fuses into helium.  The reaction produces a tremendous amount of energy that we see as light.
640432
The Hertzsprung-Russell diagram was developed based on the independent work of the 2 astronomers Henry Norris Russell and Ejnar Hertzsprung in the late 1800s.\n\nThey were investigating the luminosity and spectral class of stars.  The luminosity of a star is the total energy output of the star across all wavelengths (actually the bolometric luminosity).
772178
http://en.wikipedia.org/wiki/Astronomers
149440
http://www.chemicalelements.com/elements/k.html\n\nhttp://www-spof.gsfc.nasa.gov/stargaze/Q6.htm
467873
This isn't in the form of a graph, but it might help -->http://www.cosmobrain.com/cosmobrain/res/nearstar.html
993719
I did the same study myself last semester and didn't find much either.  If you have something specific you are looking for, Wikipedia may have it.  Also, if you don't mind looking at scientific literature try google scholar or your local university library journals.  That is where I had to get most of my stuff.  Sorry...  and Good Luck!
227515
For lower mass stars like the sun they are powered by a fusion sequence known as the proton-proton chain.\n\nThe main chain of it (there are actually three variations!) goes along the lines of:\n\nStep #1  Two hydrogen nuclei (protons) undergo fusion and beta decay to produce a positron, a neutrino, and a mass-2 isotope of hydrogen (deuterium).\n\nStep #2 The deuterium reacts with another hydrogen nuclei (a proton) to produce Helium-3 and a gamma-ray.\n\nStep #3 Two helium-3 isotopes produced in separate implementations of steps (1) and (2) fuse to form a Helium-4 nucleus plus two protons.\n\nThe net result of this is that 4H -> He + energy.  The gamma rays and the resulting matter-antimatter anihilation of the positron all produce energy to drive the sun's luminosity.\n\nFor simlicity's sake I've excluded the neutrinos, as they only matter to the energy budget when you look at the reaction in extra fine detail.
1165787
Try this:\nhttp://www.braeunig.us/space/
935563
Try http://heasarc.gsfc.nasa.gov/docs/snr.html \nand   http://en.wikipedia.org/wiki/Supernova\n\nalso try www.nasa .gov
60319
http://www2.naic.edu/~gibson/pleiades/
961557
The stars emit particles that reach us.
711840
http://www.cosmicordering.net/\nhere ya go.
104087
Have a look here,\nhttp://outreach.physics.utah.edu/labs/star_life/starlife_main.html
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Space Science Telescope Institute\nhttp://www.stsci.edu/resources/