'Star 2' presentation slideshows

The First DIRECT Distance to M33

The First DIRECT Distance to M33. Alceste Bonanos Carnegie - DTM March 8 th , 2006. Collaborators. Kris Stanek Tom Matheson Rolf Kudritzki Barbara Mochejska Lucas Macri Norbert Przybilla Dimitar Sasselov Andrew Szentgyorgyi

732 views • 62 slides

KEYSTONE STARS FINANCIAL AWARDS PROGRAM

569 views • 40 slides

2012 Implementation: A QUALITYstarsNY Recruitment Workshop

2012 Implementation: A QUALITYstarsNY Recruitment Workshop. Goals. Increase your understanding of QUALITYstarsNY Answer your questions and concerns about participating in QUALITYstarsNY Have you apply to participate!. Agenda. Welcome What is QUALITYstarsNY? The implementation process

413 views • 34 slides

544 views • 33 slides

2012 Implementation :

2012 Implementation :. A QUALITYstarsNY Recruitment Session. Goals. Increase your understanding of QUALITYstarsNY Answer your questions and concerns about participating in QUALITYstarsNY Have you apply to participate!. Agenda. Welcome What is QUALITYstarsNY? The implementation process

408 views • 33 slides

Star Inner Tracking upgrade

Star Inner Tracking upgrade. F. Videbaek STAR collaboration for the HFT upgrade group. Overview. Physics Goals for Heavy Flavour Tracker (HFT) Overview of STAR Expected Physics Results (Simulations) Detector Components for HFT Pixel IST SSD Infrastructure Summary. Physics Goals.

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Three types of binary stars.

422 views • 31 slides

II-6 Stellar Mass and Binary Stars (Main Ref.: Lecture notes;

Lec. 5. II-6 Stellar Mass and Binary Stars (Main Ref.: Lecture notes; FK Sec.4 - 4, 6, 7; 17-9, 10, and 11, Box 4-2, 4-4) II-6a. Introduction If the star is isolated, hard to measure mass directly.

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KEYSTONE STARS FINANCIAL AWARDS PROGRAM

326 views • 18 slides

Photometry with technique of Template Subtraction: personal experience .

299 views • 18 slides

456 views • 16 slides

Space Distances using Parallax

Analyze and Conclude. Your mission is to find the distance to the light bulb star in the classroom using the parallax shift in a model telescope. Q2. Was your prediction in Step 12 correct? Why or why not? Q3. How did your calculation for Star 1 compare with the actual distance?

211 views • 3 slides