Be星 (Chinese Wikipedia)

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Rivinius, Thomas; Carciofi, Alex C.; Martayan, Christophe. Classical Be stars. The Astronomy and Astrophysics Review. 2013, 21 (1): 69. Bibcode:2013A&ARv..21...69R. ISSN 0935-4956. S2CID 118652497. arXiv:1310.3962 . doi:10.1007/s00159-013-0069-0.

Porter, John M.; Rivinius, Thomas. Classical Be Stars. Publications of the Astronomical Society of the Pacific. 2003, 115 (812): 1153. Bibcode:2003PASP..115.1153P. doi:10.1086/378307 .
Rivinius, Thomas; Carciofi, Alex C.; Martayan, Christophe. Classical Be stars. The Astronomy and Astrophysics Review. 2013, 21 (1): 69. Bibcode:2013A&ARv..21...69R. ISSN 0935-4956. S2CID 118652497. arXiv:1310.3962 . doi:10.1007/s00159-013-0069-0.
Secchi, A. Schreiben des Herrn Prof.Secchi, Dir. Der Sternwarte des Collegio Romano, an den Herausgeber. Astronomische Nachrichten. 1867, 68 (4): 63–64 [2023-05-17]. Bibcode:1866AN.....68...63S. doi:10.1002/asna.18670680405. （原始内容存档于2023-05-17）.
Merrill, P. W.; Humason, M. L.; Burwell, C. G. Discovery and Observations of Stars of Class Be. Astrophysical Journal. 1925, 61: 389. Bibcode:1925ApJ....61..389M. doi:10.1086/142899.
Snow, T. P.; Marlborough, J. M. Evidence for mass loss at moderate to high velocity in Be stars. Astrophysical Journal. 1976, 203: L87. Bibcode:1976ApJ...203L..87S. doi:10.1086/182025.
Massa, D. The influence of rotation and stellar winds upon the Be phenomenon. Astronomical Society of the Pacific. 1975, 87: 777. Bibcode:1975PASP...87..777M. doi:10.1086/129842 .
Struve, Otto. On the Origin of Bright Lines in Spectra of Stars of Class B. Astrophysical Journal. 1931, 73: 94. Bibcode:1931ApJ....73...94S. doi:10.1086/143298.

Porter, John M.; Rivinius, Thomas. Classical Be Stars. Publications of the Astronomical Society of the Pacific. 2003, 115 (812): 1153. Bibcode:2003PASP..115.1153P. doi:10.1086/378307 .
Rivinius, Thomas; Carciofi, Alex C.; Martayan, Christophe. Classical Be stars. The Astronomy and Astrophysics Review. 2013, 21 (1): 69. Bibcode:2013A&ARv..21...69R. ISSN 0935-4956. S2CID 118652497. arXiv:1310.3962 . doi:10.1007/s00159-013-0069-0.
Secchi, A. Schreiben des Herrn Prof.Secchi, Dir. Der Sternwarte des Collegio Romano, an den Herausgeber. Astronomische Nachrichten. 1867, 68 (4): 63–64 [2023-05-17]. Bibcode:1866AN.....68...63S. doi:10.1002/asna.18670680405. （原始内容存档于2023-05-17）.
Merrill, P. W.; Humason, M. L.; Burwell, C. G. Discovery and Observations of Stars of Class Be. Astrophysical Journal. 1925, 61: 389. Bibcode:1925ApJ....61..389M. doi:10.1086/142899.
Snow, T. P.; Marlborough, J. M. Evidence for mass loss at moderate to high velocity in Be stars. Astrophysical Journal. 1976, 203: L87. Bibcode:1976ApJ...203L..87S. doi:10.1086/182025.
Massa, D. The influence of rotation and stellar winds upon the Be phenomenon. Astronomical Society of the Pacific. 1975, 87: 777. Bibcode:1975PASP...87..777M. doi:10.1086/129842 .
Struve, Otto. On the Origin of Bright Lines in Spectra of Stars of Class B. Astrophysical Journal. 1931, 73: 94. Bibcode:1931ApJ....73...94S. doi:10.1086/143298.

Rivinius, Thomas; Carciofi, Alex C.; Martayan, Christophe. Classical Be stars. The Astronomy and Astrophysics Review. 2013, 21 (1): 69. Bibcode:2013A&ARv..21...69R. ISSN 0935-4956. S2CID 118652497. arXiv:1310.3962 . doi:10.1007/s00159-013-0069-0.

Rivinius, Thomas; Carciofi, Alex C.; Martayan, Christophe. Classical Be stars. The Astronomy and Astrophysics Review. 2013, 21 (1): 69. Bibcode:2013A&ARv..21...69R. ISSN 0935-4956. S2CID 118652497. arXiv:1310.3962 . doi:10.1007/s00159-013-0069-0.