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.Phil. & .The. Protostars: The 1990’s Retrospective

Explore the groundbreaking Phil. & The Protostars project from the 1990s involving a plethora of prominent astronomers and researchers like Campbell, O’Neal, Casey, Jones, Feigelson, and many more. This retrospective showcases the evolution of studying protostars amidst collaborations and advancements in the field. Join us in unraveling the intricate web of research and discoveries that shaped the astronomical community during this era.

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.Phil. & .The. Protostars: The 1990’s Retrospective

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  1. Phil & The Protostars:The 1990’s Restrospective Ned Ladd Bucknell University

  2. There’s Campbell and O’Neal and Casey, Jones and Feigelson, Padman, Wooten, Ho, and Thaddeus and Cameron, Bergin, Dore, Gammie, di Francesco, Wood, and Davidson, And Welser, Henkel, Williams, Fuller, Barnes, Lee and Gregerson. Ohashi, Shaff, Garay, Burkert, Evans, yes and Claussen Bachiller, Terebey, Bastien, eh, Kazes, Lada, Clayton Kastner, Moran, Vogel, Harper, Goldsmith, Langer, Wilson And Heyer, Vrba, Walter, Brown, Welch, Plume, and Lazarian. There’s Wilner, Adams, Walmsley, and Caselli, Benson, Troland, Crutcher, Heiles, Wilking, Ladd, and Clemens, Guilloteau, Mathieu, Maradones, (phew!), and Camenzind And Grenfell, Hughes, Kane and Greene, Hujeirat and Goodman. Tafalla, Jijina, Codella, Chen, Hoeflich, Menard, Thank God I’m done with the list, ‘cuz it was really hard, These are the folks who with the ‘90’s Phil co-starred, While he worked hard in his spot not far from Harvard Yard.

  3. Does the Shu Fit?

  4. The Frequent Flyer Grad Program

  5. Does the Shu Fit?

  6. Resolving Issues

  7. The Antidote to Parameter Proliferation

  8. I’ll Have BLT (Diagram) To Go Chen et al. 1995

  9. Or Just Make One at Home Myers, Adams, Chen & Schaff 1998

  10. Comparing Nurseries Chen et al. 1997

  11. It’s Getting Crowded Out There Tafalla et al. 2000 (top); Williams & Myers 2000 (bottom)

  12. Through the “Middle Ages” to Y2K: Where We Were Individual Sources  Multiple Source Surveys Properties of Protostars  Properties of Complexes Isolated Formation  External Influences

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