单词 | pre-main-sequence |
释义 | > as lemmaspre-main-sequence pre-main-sequence adj. Brit. /ˌpriːmeɪnˈsiːkw(ə)ns/ , U.S. /ˌpriˌmeɪnˈsikwəns/ Astronomy designating a star which is too young (and therefore too bright, hot, or small) to belong to the main sequence on a Hertzsprung-Russell diagram; cf. main adj.2ΚΠ 1958 M. Schwarzschild Structure & Evol. Stars iv. 156 The pre-main-sequence phases of stellar evolution represent the contraction of a stellar mass from the state of an interstellar cloud to the initial main-sequence state. 1964 Science 20 Nov. 1032/2 E. Schatzman discusses the pre-main sequence stages in great theoretical detail. 1979 C. Payne-Gaposchkin Stars & Clusters iii. 44 Pre-main-sequence stars are gravitationally fed; main-sequence stars are devouring hydrogen. 2003 Economist (Nexis) 22 Nov. An astronomer, presumably with a sense of humour, named this type of object a PMS (pre-main sequence) star. HD 100546 has not yet started ‘burning’ hydrogen. < as lemmas |
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