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Analyzing Globular Clusters

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Presentation on theme: "Analyzing Globular Clusters"— Presentation transcript:

1

2 Analyzing Globular Clusters
Minyoung Jang Elise Pasoreck Shankar Iyer

3 A Sample Hertzsprung-Russell Diagram

4 M13—V Filter Image M13—B Filter Image

5

6 T(kK) = (12.88)(CI + 1)-1.61 kiloKelvins
tavg(years) = ( x 1028)T-4.93 years Range: 926 million – 5.44 billion TwinJet Nebula

7 Jedi Masters

8 Pluto and the Cosmological Constant
Doug Swanson, Sheila Prakash, Vicky Lent

9 History of the Cosmological Constant
Concept developed in 1917 by Einstein to make the universe static Cosmological constant (Λ) initially negative Discarded in 1929 after Hubble discovered the red shift of distant galaxies However, recent evidence indicates Λ may exist, but with positive value

10 Every object in the universe should be affected by Λ
Since Pluto is the farthest easily measured object from the Sun, we chose it to observe

11 Procedure Λ < 8.51 x 10-62 rad2/kg
Took 4 exposures of Pluto from 7/31 to 8/6 Aligned pictures with imaging software Measured Pluto’s linear and angular velocity (ω) Calculated upper limit for cosmological constant Λ < 8.51 x rad2/kg

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13 Crescent Nebula

14 What elements are in the star?
Project Vega What elements are in the star? Abigail Huang Gary Yen

15 Self Guided Spectrometer
Pick up your diffraction gratings!

16 Spectra!

17 Vega Spectrum

18 Wavelengths of Spectral Lines
Accepted (A) 3889 HI 3934 Ca K 3970 HI 4861 HI 5169 FeII 6562 HI 6869 O2 Experimental (A) 3350 HI 3660 Ca K 3930 HI 4860 HI 5170 FeII 6570 HI 6830 O2 % Error -13.9% -6.96% -1.01% reference 0.0193% -0.568% Total Error: -4.48%

19 Project Vega Successful collection of spectrum -4.48% error of lines
Vega – H(I), Ca, Fe(II),O2 Horsehead Nebula

20 Cone Nebula

21 Mark Saigh Chang Kim

22 Powered by Supermassive Black Hole
What is a Quasar? A Type of Active Galaxy Powered by Supermassive Black Hole

23 Can You Identify the Quasar
in This Field of View? (Fuhgetaboutit!)

24 How to Identify a Quasar
Look for a Redshift

25 How to Identify a Quasar (continued)
Broad Emission Lines Few Absorption Lines

26 3C345: Our Quasar You may notice that 3C345 is quite atypical, not only in its brightness, but also in its appearance:

27 Quasar 3C345 Right Ascension: 16h 42´58´
Variable Magnitude of 15 to 17 Declination: +39º 48´36" Detected Redshift: 0.595 39º 48´36"

28 Obtained Spectral Data
Spectral Lines of Quasar 3C345 Compared to That of Mercury Wavelength vs. Intensity Spectral Graph

29 Analysis Broad Absorption Lines
Not Comparable to a Typical Quasar Spectrum Not Stellar in Nature A Galactic Object or an Atypical Quasar

30 Conclusion High Magnitude and Low Redshift: Relatively Close to Earth
Not as Old as Typical Quasar Might Mean 3C345 is in Process of Evolving into Active Galaxy

31 Conclusions Age of the Milky Way ≈ 5.44 billion years
Λ < 8.51 x rad2 / kg Vega is composed of: H(I), Ca, Fe(II), O2 Quasar 3C345 is evolving into an active galaxy.

32 Acknowledgements We would like to thank the following institutions and people for enabling us to conduct this research: The State of New Jersey Drew University Dr. David Miyamoto Dr. Keith Andrew Karen Mooney


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