Lectures On Stellar Statistics
Lectures On Stellar Statistics
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In our eReader you can find the full English version of the book. Read Lectures On Stellar Statistics Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Lectures On Stellar Statistics
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22 | -3. 0 |Map | 3. 06 ||17|Fomalhaut | 0. 37| + 1. 41| 1. 29 | +0. 4 |A3 | 1. 43 ||18|Deneb | 0. 00| - 0. 84| 1. 33 | . . |A2 | 1. 42 ||19|Regulus | 0. 25| . . | 1. 34 | -2. 7 |B8 | 1. 25 ||20|β Crucis | 0. 06| + 2. 74| 1. 50 | -5. 6 |B1 | 1. 09 |+--+---------------------+------+--------+---------+---------+----+------+| | | | | | | | _m′_ || | Mean | 0″. 56| 3. 26| +0m. 64 | -2m. 1 |F1 |+1. 13 |+--+---------------------+------+--------+---------+---------+----+------+ The values of (αδ), _m_..., _Sp_ are taken from H. 50. The values of _l_, _b_ are computed from (αδ) with the help of tables in preparation at theLund Observatory, or from the original to plate I at the end, allowingthe conversion of the equatorial coordinates into galactic ones. Thevalues of π are generally taken from the table of KAPTEYN and WEERSMAmentioned in the previous chapter. The values of μ are obtained from B. P. C. , those of the radial velocity (_W_) from the card catalogue inLund already described.
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To quickly assess the difficulty of the text, read a short excerpt:
22 | -3. 0 |Map | 3. 06 ||17|Fomalhaut | 0. 37| + 1. 41| 1. 29 | +0. 4 |A3 | 1. 43 ||18|Deneb | 0. 00| - 0. 84| 1. 33 | . . |A2 | 1. 42 ||19|Regulus | 0. 25| . . | 1. 34 | -2. 7 |B8 | 1. 25 ||20|β Crucis | 0. 06| + 2. 74| 1. 50 | -5. 6 |B1 | 1. 09 |+--+---------------------+------+--------+---------+---------+----+------+| | | | | | | | _m′_ || | Mean | 0″. 56| 3. 26| +0m. 64 | -2m. 1 |F1 |+1. 13 |+--+---------------------+------+--------+---------+---------+----+------+ The values of (αδ), _m_..., _Sp_ are taken from H. 50. The values of _l_, _b_ are computed from (αδ) with the help of tables in preparation at theLund Observatory, or from the original to plate I at the end, allowingthe conversion of the equatorial coordinates into galactic ones. Thevalues of π are generally taken from the table of KAPTEYN and WEERSMAmentioned in the previous chapter. The values of μ are obtained from B. P. C. , those of the radial velocity (_W_) from the card catalogue inLund already described.
What to read after Lectures On Stellar Statistics?
You can find similar books in the "Read Also" column, or choose other free books by Charlier Carl Vilhelm Ludvig to read onlineMoreLess
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