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My Fraternity Room
 
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Views: 1142 Bradley Allen
how to make chocolate garnishes decorations tutorial PART 2 how to cook that ann reardon
 
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How to make chocolate decorations to garnish your desserts. Part 2 For video on how to temper chocolate: http://youtu.be/s2aPf1wSjds For template for piped designs: http://www.howtocookthat.net/public_html/chocolate-decorations-for-desserts/ To buy the texture mats that I used: http://www.amazon.com/gp/product/1591741947/ref=as_li_qf_sp_asin_tl?ie=UTF8&tag=howtocookthat-20&linkCode=as2&camp=1789&creative=9325&creativeASIN=1591741947 These beautiful chocolate garnishes and chocolate decorations are perfect to put on top of any cake or dessert. So easy and impressive. How to Cook That is a dessert cooking channel with step by step video tutorials for yummy desserts, macarons, cupcakes, chocolate and cake decorating lessons. For printable copies of the recipes visit the website at http://www.howtocookthat.net SUBSCRIBE : http://www.youtube.com/subscription_center?add_user=howtocookthat CHOCOLATE TUTORIALS: http://www.youtube.com/watch?v=BkIvy9Hz8r0&list=SP2D2F4E4B08214BC2 DESSERT RECIPES: http://www.youtube.com/watch?v=t3Ur6IRgAxw&list=PL568F5B0E018FF937 CAKE DECORATING LESSONS: http://www.youtube.com/watch?v=6mGkcynKQBc&list=PL2639AB7064048F68&feature=plcp CAKE POPS AND MACARON: http://www.youtube.com/watch?v=qS4DJgFmNFM&list=PL2FB2964D0EFB635B&feature=view_all Business enquiries only: howtocookthat [at] iinet.net.au SEND MAIL TO: Ann Reardon PO Box 202 Chirnside Park LPO Australia 3116
Views: 6807136 How To Cook That
How to Ask Your Date to Formal
 
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Sean Rice and Matt Cosenzo from the Lambda Tau Chapter of the Sigma Chi fraternity asked their dates to Formal with a video. Enjoy! song list- Blue ( da ba dee) - Eiffel 65 cuban pete - the mask soundtrack wanted - Hunter Haze Take me there - Rascal Flatts Better Together - Jack Johnson
Views: 5043 Sean Rice
What's Lavalier All About?
 
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We're so excited to release our first teaser video! This video was inspired to show you what we're all about! We at Lavalier want to give the best to the Sorority Bride & Fraternity groom. From your lavaliering to your post wedding fun we'll make sure you have the best inspiration, tips, tricks, & knowledge to make these important experience worth remembering! Alongside that we've paired the absolute best vendors in your areas to make sure no matter where you are we've got you covered on your big day! Go to our vendies list at www.lavaliermagazine.com/vendies to find the best vendors for your day! Enjoy this AXO inspired photoshoot that shows a wedding orchestrated with the help of Lavalier. We found all the vendors from venue to dress to help these UH AXO girls! Stay tuned for more videos from the Lavalier Team!
Views: 106 Lavalier Magazine
School Board Says Family Ties Allowed Store Owner To Sell Alcohol Near School
 
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A number of residents say they believe a store owner's family ties are allowing him the advantage of selling alcohol near a school, against the wishes of police and the school district. Rachel Kim reports.
Views: 482 CBS Los Angeles
Sorority Rush OOTD!!
 
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Views: 1970 collegeamore
Smash my bunk bed
 
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Views: 89 team lebron
Stellar classification | Wikipedia audio article | Wikipedia audio article
 
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This is an audio version of the Wikipedia Article: Stellar classification | Wikipedia audio article Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago. Learning by listening is a great way to: - increases imagination and understanding - improves your listening skills - improves your own spoken accent - learn while on the move - reduce eye strain Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone. You can find other Wikipedia audio articles too at: https://www.youtube.com/channel/UCuKfABj2eGyjH3ntPxp4YeQ In case you don't find one that you were looking for, put a comment. This video uses Google TTS en-US-Standard-D voice. SUMMARY ======= In astronomy, stellar classification is the classification of stars based on their spectral characteristics. Electromagnetic radiation from the star is analyzed by splitting it with a prism or diffraction grating into a spectrum exhibiting the rainbow of colors interspersed with spectral lines. Each line indicates a particular chemical element or molecule, with the line strength indicating the abundance of that element. The strengths of the different spectral lines vary mainly due to the temperature of the photosphere, although in some cases there are true abundance differences. The spectral class of a star is a short code primarily summarizing the ionization state, giving an objective measure of the photosphere's temperature. Most stars are currently classified under the Morgan-Keenan (MK) system using the letters O, B, A, F, G, K, and M, a sequence from the hottest (O type) to the coolest (M type). Each letter class is then subdivided using a numeric digit with 0 being hottest and 9 being coolest (e.g. A8, A9, F0, and F1 form a sequence from hotter to cooler). The sequence has been expanded with classes for other stars and star-like objects that do not fit in the classical system, such as class D for white dwarfs and classes S and C for carbon stars. In the MK system, a luminosity class is added to the spectral class using Roman numerals. This is based on the width of certain absorption lines in the star's spectrum, which vary with the density of the atmosphere and so distinguish giant stars from dwarfs. Luminosity class 0 or Ia+ is used for hypergiants, class I for supergiants, class II for bright giants, class III for regular giants, class IV for sub-giants, class V for main-sequence stars, class sd (or VI) for sub-dwarfs, and class D (or VII) for white dwarfs. The full spectral class for the Sun is then G2V, indicating a main-sequence star with a temperature around 5,800 K.
Views: 0 wikipedia tts
Late-type star | Wikipedia audio article | Wikipedia audio article
 
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This is an audio version of the Wikipedia Article: Late-type star | Wikipedia audio article Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago. Learning by listening is a great way to: - increases imagination and understanding - improves your listening skills - improves your own spoken accent - learn while on the move - reduce eye strain Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone. You can find other Wikipedia audio articles too at: https://www.youtube.com/channel/UCuKfABj2eGyjH3ntPxp4YeQ You can upload your own Wikipedia articles through: https://github.com/nodef/wikipedia-tts "The only true wisdom is in knowing you know nothing." - Socrates SUMMARY ======= In astronomy, stellar classification is the classification of stars based on their spectral characteristics. Electromagnetic radiation from the star is analyzed by splitting it with a prism or diffraction grating into a spectrum exhibiting the rainbow of colors interspersed with spectral lines. Each line indicates a particular chemical element or molecule, with the line strength indicating the abundance of that element. The strengths of the different spectral lines vary mainly due to the temperature of the photosphere, although in some cases there are true abundance differences. The spectral class of a star is a short code primarily summarizing the ionization state, giving an objective measure of the photosphere's temperature. Most stars are currently classified under the Morgan-Keenan (MK) system using the letters O, B, A, F, G, K, and M, a sequence from the hottest (O type) to the coolest (M type). Each letter class is then subdivided using a numeric digit with 0 being hottest and 9 being coolest (e.g. A8, A9, F0, and F1 form a sequence from hotter to cooler). The sequence has been expanded with classes for other stars and star-like objects that do not fit in the classical system, such as class D for white dwarfs and classes S and C for carbon stars. In the MK system, a luminosity class is added to the spectral class using Roman numerals. This is based on the width of certain absorption lines in the star's spectrum, which vary with the density of the atmosphere and so distinguish giant stars from dwarfs. Luminosity class 0 or Ia+ is used for hypergiants, class I for supergiants, class II for bright giants, class III for regular giants, class IV for sub-giants, class V for main-sequence stars, class sd (or VI) for sub-dwarfs, and class D (or VII) for white dwarfs. The full spectral class for the Sun is then G2V, indicating a main-sequence star with a temperature around 5,800 K.
Views: 5 wikipedia tts