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Relative Strengths of Absorption Lines lonized Neutral Hydrogen helium helium lonized metals Neutral Molecules (TiO) metals B F Spectral Class M >30,000 10,000 7500- 30,000 6000- 5200- 3700- 10,000 7500 6000 2400- 5200 3700 Approximate Temperature (K) According to the graph shown above, for which spectral class stars are the following absorption lines the strongest? Neutral Metals [Select] Hydrogen [Select] Neutral Helium [Select]

Relative Strengths of Absorption Lines lonized Neutral Hydrogen helium helium lonized metals Neutral Molecules (TiO) metals B F Spectral Class M >30,000 10,000 7500- 30,000 6000- 5200- 3700- 10,000 7500 6000 2400- 5200 3700 Approximate Temperature (K) According to the graph shown above, for which spectral class stars are the following absorption lines the strongest? Neutral Metals [Select] Hydrogen [Select] Neutral Helium [Select]

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Relative Strengths of Absorption Lines lonized Neutral Hydrogen helium helium lonized metals Neutral Molecules (TiO) metals B A F G K M Spectral Class >30,000 10,000- 7500- 30,000 6000- 5200- 10,000 7500 6000 Approximate Temperature (K) 3700- 2400- 5200 3700 According to the graph shown above, for which spectral class stars are the following absorption lines the strongest? Neutral Metals [Select] Hydrogen [Select] Neutral Helium [Select]
Transcribed Image Text:Relative Strengths of Absorption Lines lonized Neutral Hydrogen helium helium lonized metals Neutral Molecules (TiO) metals B A F G K M Spectral Class >30,000 10,000- 7500- 30,000 6000- 5200- 10,000 7500 6000 Approximate Temperature (K) 3700- 2400- 5200 3700 According to the graph shown above, for which spectral class stars are the following absorption lines the strongest? Neutral Metals [Select] Hydrogen [Select] Neutral Helium [Select]
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