Adelman, S. Et Al. 1997. Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY , no.2 , 470-500.

Adelman, S., Caliskan, H., Kocer, D., & Bolcal, C., (1997). Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY , no.2, 470-500.

Adelman, SJ Et Al. "Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii," MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY , no.2, 470-500, 1997

Adelman, SJ Et Al. "Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii." MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY , no.2, pp.470-500, 1997

Adelman, S. Et Al. (1997) . "Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii." MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY , no.2, pp.470-500.

@article{article, author={SJ Adelman Et Al. }, title={Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii}, journal={MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY}, year=1997, pages={470-500} }