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Lessons from the. Illustris Simulation . Shy . Ge...
An X-ray/UV Perspective. Edmund Hodges-. Kluck. Jo...
at High Redshift Universe. KenTaro. Motohara . (....
Metallicity. Relation at High . Redshifts. Stell...
Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve ....
Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve ....
metallicity. gradients . in disk galaxies from ....
Dana . Balser. (NRAO) . Loren Anderson (WVU), To...
Lisa Kewley. Australian National University. Thank...
David Spergel. What has changed?. Context:. Standa...
/Fe]. SNII . release. . most. . alpha. –. ele...
stars. T. . Sivarani. . Indian Institute of Astr...
Planet-Host Stars. 2013. 2. 22. . Wonseok. Kang ...
“Stars in transition”. Caroline Roberts. Pola...
metallicity. on pulsating B stars in the LMC (. ...
. CDM Cosmology. Oleg . Gnedin. (University of...
50 years of Wide Field Studies, La Serena, 5/2013...
Patricia . Sánchez-Blázquez. (UAM). Jairo. Me...
Low-. Redshift. Galaxies. Adam Leroy (NRAO, Nor...
Adam Leroy. National Radio Astronomy Observatory....
Diane Feuillet . New Mexico State University. Jon...
Steve . Goldman. 12 April, 2016. Cavendish Labora...
Metallicity. Stellar Abundances: Victories and S...
Laura . Magrini. INAF- . Osservatorio. . Astrofis...
Ultra Metal - Poor (UMP ; [Fe/H] - 4 . 0 ) stars h...
![[C II ] is an important SF tracer in particularly in low-metallicity environments, because of la](https://thumbs.docslides.com/916757/c-ii-is-an-important-sf-tracer-in-particularly-in-low-metallicity-environments-because-of-la.jpg)
SOFIA [C . II. ]158 . μ. m vs H . I, . and ...
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