grb absorption spectroscopy - Inaf

Recommendations

Info

GRB 050730 Second component: UV pumping scenario favoured G/G0 = 105 ÷ 106 where G0 = 1.6 X 10-3 erg cm-2 s-1 . Third component: possibly electron-ion collisions at work From C II fine structure doublet: 10 3 < T< 10 4 K 10 < n e < 60 cm -3
Page 1 and 2: Absorption studies of GRB afterglow
Page 3 and 4: Suitable to: GRB ABSORPTION SPECTRO
Page 5 and 6: LOW - RES GRBs GRBs provide an inde
Page 7 and 8: Advantages: Piranomonte et al. 2008
Page 9 and 10: FINE STRUCTURE FEATURES The gross s
Page 11: GRB 060418: VARIABILITY Fine struct
Page 14 and 15: CrII groud state line is decreasing
Page 18 and 19: OVI Lyβ SII NiII NV NiII Lyα OI/S
Page 20 and 21: MAIN SYSTEM METALLICITY Ly_α Missi
Page 26 and 27: CONCLUSIONS GRBs are a new tool to
Page 28 and 29: GRB explosion site Host gas far awa
Page 32 and 33: GRB 050730 The main system presents
Page 34 and 35: GRB 050730 Fine structure transitio
Page 38 and 39: 1) 2) 3) 5) 4) Unidentified Main In
Page 40 and 41: GRB080319B - MAIN SYSTEM: COMPONENT
Page 42 and 43: GRB080319B - FINE STRUCTURE LINE VA
Page 44 and 45: Balance equation: dN t u dt ( ) TIM
Page 47 and 48: GRB080330 - MAIN SYSTEM: COMPONENTS
Page 49: GRB080330 - TIME DEPENDENT MODELING
Page 52 and 53: INTERVENING ABSORBERS GRB080319B NO
Page 54: THE GRB090926A SIGHTLINE Four, very

grb absorption spectroscopy - Inaf

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?