Zobrazeno 1 - 10
of 192
pro vyhledávání: '"Anne B. Underhill"'
Autor:
McNally, D.
Publikováno v:
Science Progress (1933- ), 1967 Oct 01. 55(220), 631-632.
Externí odkaz:
https://www.jstor.org/stable/43419699
Autor:
Lawrence H. Aller
Publikováno v:
Science. 156:785-785
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b95aed3cded1a5414d18b06434e63713
https://doi.org/10.1126/science.156.3776.785.b
https://doi.org/10.1126/science.156.3776.785.b
Autor:
Anne B. Underhill
Publikováno v:
Astrophysics and Space Science. 221:383-389
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::278d257f6ffef194f0a08e77937f8d1b
https://doi.org/10.1007/bf01091169
https://doi.org/10.1007/bf01091169
Autor:
Anne B. Underhill, Grant M. Hill
Publikováno v:
Space Science Reviews. 66:281-284
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7094b2f5ca7a1e05bc10df1b7aa30ecf
https://doi.org/10.1007/bf00771078
https://doi.org/10.1007/bf00771078
Autor:
Anne B. Underhill
Publikováno v:
Symposium - International Astronomical Union. 143:53-58
The evidence is reviewed that Population I Wolf-Rayet stars have solar abundances, that they are surrounded by remnant disks formed from their natal clouds, and that their rate of mass loss is moderate. These properties are consistent with Wolf-Rayet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0b43f7db4783f990fee5107ce167707d
https://doi.org/10.1017/s0074180900044867
https://doi.org/10.1017/s0074180900044867
Autor:
Anne B. Underhill
Publikováno v:
Cool Stars, Stellar Systems, and the Sun ISBN: 9783540129073
The physical state of the mantle of a star (its chromosphere, corona, and wind) is chiefly determined by the amount of nonradiative heat and momentum deposited in the mantle. Because the presence of magnetic lines of force buffeted by turbulent or co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::326ed464fd8d762839ca583c6d52dfc8
https://doi.org/10.1007/3-540-12907-3_208
https://doi.org/10.1007/3-540-12907-3_208
Autor:
Anne B. Underhill
Publikováno v:
Astrophysics and Space Science Library ISBN: 9789401061759
I first met Edith Muller in connection with my studies of the theories and observations of the spectra of massive stars and her related studies of the spectrum of the Sun. Later I was well aware of her work as General Secretary of the International A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5442780ee82a6cff5d7ccd0bb6f0c47c
https://doi.org/10.1007/978-94-011-5173-3_30
https://doi.org/10.1007/978-94-011-5173-3_30
Autor:
Anne B. Underhill
Publikováno v:
Angular Momentum and Mass Loss for Hot Stars ISBN: 9789401074469
Wolf-Rayet Stars and Interrelations with other Massive Stars in Galaxies ISBN: 9780792310877
Wolf-Rayet Stars and Interrelations with other Massive Stars in Galaxies ISBN: 9780792310877
The fundamental properties of the Wolf-Rayet components of V444 Cygni and CQ Cephei such as mass, effective temperature, and luminosity are presented. These properties are consistent with these stars being young objects recently arrived on the main s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e84c02669a17206ff0a085ab7a5b2f51
https://doi.org/10.1007/978-94-009-2105-4_33
https://doi.org/10.1007/978-94-009-2105-4_33
Autor:
Anne B. Underhill
Publikováno v:
Angular Momentum and Mass Loss for Hot Stars ISBN: 9789401074469
The evidence is reviewed that Population I Wolf-Rayet stars have solar abundances, that they are surrounded by remnant disks formed from their natal cloud, and that their rate of mass loss is moderate. These properties are consistent with Wolf-Rayet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ae3309a6b29d5553bd18f3f7fbe6dd80
https://doi.org/10.1007/978-94-009-2105-4_8
https://doi.org/10.1007/978-94-009-2105-4_8