1. Experimental Results for H2 Formation from H- and H and Implications for First Star Formation Kreckel, H.; Bruhns, H.; Čížek, M.; Glover, S. C. O.; Miller, K. A.; Urbain, X.; Savin, Daniel Wolf 2010 Articles AstrophysicsPhysics
2. Molecular Hydrogen Formation in the Early Universe: New Implications From Laboratory Measurements Savin, Daniel Wolf; Miller, Kenneth; Kreckel, H.; Bruhns, H.; Urbain, X.; Glover, S. C. O.; Cizek, M. 2010 Presentations (Communicative Events) AstrophysicsPlasma (Ionized gases)Physics
3. Complete tables: Is H3+ cooling ever important in primordial gas? Glover, S. C. O.; Savin, Daniel Wolf 2009 Articles AstrophysicsPhysics
4. Is H+3 cooling ever important in primordial gas? Glover, S. C. O.; Savin, Daniel Wolf 2009 Articles AstrophysicsMicrophysics
5. Is H+3 cooling ever important in primordial gas? Glover, S. C. O.; Savin, Daniel Wolf 2009 Data (Information) AstrophysicsPlasma (Ionized gases)PhysicsMicrophysics
6. Is H3+ cooling ever important in primordial gas? Glover, S. C. O.; Savin, Daniel Wolf 2009 Articles AstrophysicsPhysics
7. Cosmological Implications of the Uncertainty in Astrochemical Rate Coefficients Savin, Daniel Wolf; Glover, S. C. O.; Jappsen, A. K. 2006 Presentations (Communicative Events) AstrophysicsPlasma (Ionized gases)Physics
8. Cosmological Implications of the Uncertainty in H– Destruction Rate Coefficients Savin, Daniel Wolf; Glover, S. C. O.; Jappsen, A. K. 2006 Articles Astrophysics