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8.93E-24. 6.12E-11. 1.04E-09. –. 3.33E-12. 7.91E-13. 9.60E-10. Al(5s) H. 1.95E-26. 1.28E-12. 1.48E-11. 1.98E-11. –. 1.88E-11. 1.87E-11. Al(nd) H. 1.37E-29.

PDF (105.1 KB) - Astronomy & Astrophysics - Tài liệu liên quan

PDF (105.1 KB) - Astronomy & Astrophysics

8.93E-24. 6.12E-11. 1.04E-09. –. 3.33E-12. 7.91E-13. 9.60E-10. Al(5s) H. 1.95E-26. 1.28E-12. 1.48E-11. 1.98E-11. –. 1.88E-11. 1.87E-11. Al(nd) H. 1.37E-29.

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(2014) from comet 67P combined with several parameters determined from the current encounter of Rosetta with the comet. In the following section, we briefly ...

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stable over many years, and the phase of minimum light can be stable as well for several years. On the long term, ... The first photoelectric UBVR observations of these stars re- vealed periodic ... We targetted 48 WTTS for long-term mon- itoring ... TAP 9. 351. K5. 48858–49635. 3. 12.25–12.08. 82. 1.05. 0.99. VB (0. 61) le93.

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