Stothers 1968

Stothers, R., 1968: An interpretation of the peculiar helium star HZ 29. Astrophys. J., 154, L91-L94, doi:10.1086/180276.

It is suggested that the variability of the peculiar helium star HS 29 is due to nuclear-energized pulsations in a helium star of high mass.

• Download PDF (Document is 296 kB; scanned, no OCR)
• PDF documents require a special viewer such as the free Adobe Reader.

Citation Styles

Show: ACP, AGU, AMS, ApJ, JQSRT, Science style

Stothers, R.: An interpretation of the peculiar helium star HZ 29, Astrophys. J., 154, L91-L94, doi:10.1086/180276, 1968.

Stothers, R. (1968), An interpretation of the peculiar helium star HZ 29, Astrophys. J., 154, L91-L94, doi:10.1086/180276.

Stothers, R., 1968: An interpretation of the peculiar helium star HZ 29. Astrophys. J., 154, L91-L94, doi:10.1086/180276.

Stothers, R. 1968, Astrophys. J., 154, L91, doi:10.1086/180276.

Stothers R. An interpretation of the peculiar helium star HZ 29, Astrophys J 1968;154:L91-L94. doi:10.1086/180276.

R. Stothers, Astrophys. J. 154, L91-L94, doi:10.1086/180276 (1968).