From inside the book
Results 1-3 of 67
Page 367
TABLE 3 LTE Abundances in Secondary of V356 Sgr and HR 7145 с N △ ( Abundance ) HR 7145 Solarb V356 - HR7145 Abundance V356 Sgr ~ 6.5 ± 0.2 8.47 ± 0.15 8.55 9.09 ± 0.14 7.97 8.77 ± 0.21 O 8.54 ± 0.02 8.76 ± 0.07 8.87 Fe 7.18 ± 0.08 ...
TABLE 3 LTE Abundances in Secondary of V356 Sgr and HR 7145 с N △ ( Abundance ) HR 7145 Solarb V356 - HR7145 Abundance V356 Sgr ~ 6.5 ± 0.2 8.47 ± 0.15 8.55 9.09 ± 0.14 7.97 8.77 ± 0.21 O 8.54 ± 0.02 8.76 ± 0.07 8.87 Fe 7.18 ± 0.08 ...
Page 373
Table 3 LTE Abundances in Secondary of V356 Sgr and HR 7145 △ ( Abundance ) HR 7145 Solarb V356 - HR7145 Abundance V356 Sgr с ~ 6.5 ± 0.2 N 8.77 ± 0.21 8.47 ± 0.15 8.55 9.09 ± 0.14 7.97 8.76 ± 0.07 8.87 O 8.54 ± 0.02 Fe 7.18 ± 0.08 ...
Table 3 LTE Abundances in Secondary of V356 Sgr and HR 7145 △ ( Abundance ) HR 7145 Solarb V356 - HR7145 Abundance V356 Sgr с ~ 6.5 ± 0.2 N 8.77 ± 0.21 8.47 ± 0.15 8.55 9.09 ± 0.14 7.97 8.76 ± 0.07 8.87 O 8.54 ± 0.02 Fe 7.18 ± 0.08 ...
Page 373
pergiants reveals large ( 0.5-1.3 dex ) overabundances of N compared to the solar N abundance . Although the corresponding non - LTE N abundances are ~ 0.7 dex smaller than the LTE abundances , her non - LTE C and N abundances still ...
pergiants reveals large ( 0.5-1.3 dex ) overabundances of N compared to the solar N abundance . Although the corresponding non - LTE N abundances are ~ 0.7 dex smaller than the LTE abundances , her non - LTE C and N abundances still ...
What people are saying - Write a review
We haven't found any reviews in the usual places.
Other editions - View all
Common terms and phrases
abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray