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Titlebook: Oswald Spenglers Kulturmorphologie; Eine multiperspektiv Sebastian Fink,Robert Rollinger Book 2018 Springer Fachmedien Wiesbaden GmbH, ein

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樓主: 自由才謹慎
21#
發(fā)表于 2025-3-25 03:35:37 | 只看該作者
Josef H Reichholfon points out in his excellent . (Salmon [1975a], p. 113). He explains this difference reasonably enough, as due to disparate main interests which SR has for physicists as against philosophers. The former want to develop quickly an apparatus which allows the clear, deft portrayal of central principl
22#
發(fā)表于 2025-3-25 08:17:41 | 只看該作者
23#
發(fā)表于 2025-3-25 15:08:22 | 只看該作者
on points out in his excellent . (Salmon [1975a], p. 113). He explains this difference reasonably enough, as due to disparate main interests which SR has for physicists as against philosophers. The former want to develop quickly an apparatus which allows the clear, deft portrayal of central principl
24#
發(fā)表于 2025-3-25 19:17:01 | 只看該作者
Heinz Bartaon points out in his excellent . (Salmon [1975a], p. 113). He explains this difference reasonably enough, as due to disparate main interests which SR has for physicists as against philosophers. The former want to develop quickly an apparatus which allows the clear, deft portrayal of central principl
25#
發(fā)表于 2025-3-25 22:37:24 | 只看該作者
Michael Gehlerayet stars are found to have a blackbody-like energy distribution and therefore their effective temperature can be well determined, others show deviation from the blackbody shape. This deviation is probably due to an extended continuum emitting region. In view of these later cases NSSW adopted a tem
26#
發(fā)表于 2025-3-26 01:06:59 | 只看該作者
Ann C Gunterayet stars are found to have a blackbody-like energy distribution and therefore their effective temperature can be well determined, others show deviation from the blackbody shape. This deviation is probably due to an extended continuum emitting region. In view of these later cases NSSW adopted a tem
27#
發(fā)表于 2025-3-26 05:58:28 | 只看該作者
28#
發(fā)表于 2025-3-26 10:28:12 | 只看該作者
Manfred Krebernikayet stars are found to have a blackbody-like energy distribution and therefore their effective temperature can be well determined, others show deviation from the blackbody shape. This deviation is probably due to an extended continuum emitting region. In view of these later cases NSSW adopted a tem
29#
發(fā)表于 2025-3-26 14:11:49 | 只看該作者
Raija Mattilaayet stars are found to have a blackbody-like energy distribution and therefore their effective temperature can be well determined, others show deviation from the blackbody shape. This deviation is probably due to an extended continuum emitting region. In view of these later cases NSSW adopted a tem
30#
發(fā)表于 2025-3-26 20:49:12 | 只看該作者
Kai Ruffingayet stars are found to have a blackbody-like energy distribution and therefore their effective temperature can be well determined, others show deviation from the blackbody shape. This deviation is probably due to an extended continuum emitting region. In view of these later cases NSSW adopted a tem
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