Abstract
Studies in astronomy and stellar astrophysics have played a significant role in the ongoing research of the Specola Vaticana throughout its history. Within the last 150 years, this has been evidenced by the work of Angelo Secchi in the 19th century, by the Specola’s participation in the 19th–20th century Carte du Ciel project, and by the Observatory’s sponsorship of the prominent Vatican Conference on Stellar Populations in 1957. The latter was a milestone in the understanding of stellar populations. Since then, the astronomy community’s knowledge of stellar populations, especially with regard to the various components of the Milky Way Galaxy and other galaxies, along with globular and open clusters, has increased greatly, commensurate with the advent of more powerful telescopes. The Specola Vaticana continues to contribute actively to such astrophysical studies by research conducted on photometric surveys of portions of the Milky Way Galaxy and also by the study of extreme horizontal branch stars that are thought to be ubiquitous in most stellar populations.
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References
Altmann, M., de Boer, K. S., & Edelmann, H. (2001). The population membership of sdB stars: a kinematic analysis. Astronomische Nachrichten, 322, 397.
Altmann, M., Edelmann, H., & de Boer, K. S. (2004). Studying the populations of our Galaxy using the kinematics of sdB stars. Astronomy & Astrophysics, 414, 181.
Baade, W. (1944). The resolution of messier 32, NGC 205, and the central region of the andromeda nebula. The Astrophysical Journal, 100, 137.
Baschek, B., & Norris, J. (1975). The OB-type subdwarf HD 149382 and the nature of the subdwarf B stars. The Astrophysical Journal, 199, 694.
Burstein, D., Bertola, F., Buson, L. M., & Faber, S. M. (1988). The farultraviolet spectra of early-type galaxies. The Astrophysical Journal, 328, 440.
Charpinet, S., Fontaine, G., & Brassard, P., Dorman, B. 1996. The potential of asteroseismology for hot, subdwarf B stars: a new class of pulsating stars? The Astrophysical Journal, 471, L103.
D’Antona, F., & Caloi, V. 2008. The fraction of second generation stars in globular clusters from the analysis of the horizontal branch. Monthly Notices of the Royal Astronomical Society, 390, 693.
D’Cruz, N. L., Dorman, B., Rood, R. T., & O’Connell, R. W. (1996). The origin of extreme horizontal branch stars. The Astrophysical Journal, 466, 359.
Edelmann, H., Heber, U., Hagen, H.-J., Lemke, M., Dreizler, S., Napiwotzki, R., et al. (2003). Spectral analysis of sdB stars from the Hamburg Quasar Survey. Astronomy & Astrophysics, 400, 939.
Fontaine, G., Brassard, P., Charpinet, S., Green, E. M., Randall, S. K., & Van Grootel, V. (2012). A preliminary look at the empirical mass distribution of hot B subdwarf stars. Astronomy & Astrophysics, 539, A12.
Han, Z., Podsiadlowski, P., Maxted, P. F. L., Marsh, T. R., & Ivanova, N. (2002). The origin of subdwarf B stars – I. The formation channels. Monthly Notices of the Royal Astronomical Society, 336, 449.
Han, Z., Podsiadlowski, P., Maxted, P. F. L., & Marsh, T. R. (2003). The origin of subdwarf B stars – II. Monthly Notices of the Royal Astronomical Society, 341, 669.
Han, Z., Podsiadlowski, P., & Lynas-Gray, A. E. (2007). A binary model for the UV-upturn of elliptical galaxies. Monthly Notices of the Royal Astronomical Society, 380, 1098.
Groth, H. G., Kudritzki, R. P., & Heber, U. (1985). Photospheric convection zones and evolution of subluminous OB-stars. Astronomy & Astrophysics, 152, 107.
Heber, U., Hunger, K., Jonas, G., & Kudritzki, R. P. (1984). The atmosphere of subluminous B stars. Astronomy & Astrophysics, 130, 119.
Heber, U. (1986). The atmosphere of subluminous B stars. II - Analysis of 10 helium poor subdwarfs and the birthrate of sdB stars. Astronomy & Astrophysics, 155, 33.
Hu, H., Dupret, M.-A., Aerts, C., Nelemans, G., Kawaler, S. D., Miglio, A., et al. (2008). A seismic approach to testing different formation channels of subdwarf B stars. Astronomy & Astrophysics, 490, 243.
Kilkenny, D., Koen, C., O’Donoghue, D., & Stobie, R. S. (1997). A new class of rapidly pulsating star - I. EC 14026-2647, the class prototype. Monthly Notices of the Royal Astronomical Society, 285, 640.
Larsson-Leander, G. (1970). Astronomi och astrofysik. (https://commons.wikimedia.org/wiki/File:Starpop.svg).
Lee, Y.-W., Joo, S.-J., Han, S.-I., Chung, C., Ree, C.-H., Sohn, Y.-J., et al. (2005). Super-helium-rich populations and the origin of extreme horizontal-branch stars in globular clusters. The Astrophysical Journal, 621, L57.
Lisker, T., Heber, U., Napiwotzki, R., Christlieb, N., Han, Z., Homeier, D., et al. (2005). Hot subdwarfs from the ESO Supernova Ia Progenitor Survey. I. Atmospheric parameters and cool companions of sdB stars. Astronomy & Astrophysics, 430, 223.
Maxted, P. F. L., Heber, U., Marsh, T. R., & North, R. C. (2001). The binary fraction of extreme horizontal branch stars. Monthly Notices of the Royal Astronomical Society, 326, 1391.
Mengel, J. G., Norris, J., & Gross, P. G. (1976). A binary hypothesis for the subdwarf B stars. The Astrophysical Journal, 204, 488.
Moehler, S., Heber, U., & de Boer, K. S. (1990). Hot subluminous stars at high galactic latitudes. II - Physical parameters and distances of 37 sdB stars. Astronomy & Astrophysics, 239, 265.
Moni, Bidin C., Villanova, S., Piotto, G., & Momany, Y. (2011). A lack of close binaries among hot horizontal branch stars in globular clusters. II. NGC 2808. Astronomy & Astrophysics, 528, A127.
Napiwotzki, R., Karl, C. A., Lisker, T., Heber, U., Christlieb, N., Reimers, D., et al. (2004). Close binary EHB stars from SPY. Astrophysics and Space Science, 291, 321.
Newell, E. B. (1973). The evolutionary status of the blue halo stars. The Astrophysical Journal Supplement Series, 26, 37.
O’Connell, D. J. K. (ed.) (1958). Stellar Populations: Proceedings of the Conference Sponsored by the Pontifical Academy of Sciences and the Vatican Observatory.
Piotto, G., Bedin, L. R., Anderson, J., King, I. R., Cassisi, S., Milone, A. P., et al. (2007). A Triple Main Sequence in the Globular Cluster NGC 2808. The Astrophysical Journal Letters, 661, L53.
Saffer, R. A., Bergeron, P., Koester, D., & Liebert, J. (1994). Atmospheric parameters of field subdwarf B stars. The Astrophysical Journal, 432, 351.
Secchi, A. (1877). Le Stelle: Fratelli Dumolard.
Sosin, C., Dorman, B., Djorgovski, S. G., Piotto, G., Rich, R. M., King, I. R., et al. (1997). Peculiar multimodality on the horizontal branch of the globular cluster NGC 2808. The Astrophysical Journal, 480, L35.
Stroeer, A., Heber, U., Lisker, T., Napiwotzki, R., Dreizler, S., Christlieb, N., et al. (2007). Hot subdwarfs from the ESO supernova Ia progenitor survey. II. Atmospheric parameters of subdwarf O stars. Astronomy & Astrophysics, 462, 269.
Sweigart, A. V. (1997). Effects of helium mixing on the evolution of globular cluster stars. The Astrophysical Journal Supplement Series, 474, L23.
Theissen, A., Moehler, S., Heber, U., & de Boer, K.-S. (1993). Hot subluminous stars at high galactic latitudes – IV. Physical parameters and distances of 18 hot subdwarf stars and their spatial distribution. Astronomy & Astrophysics, 273, 524.
Yi, S. K., Demarque, P., & Oemler, A. J. (1998). On the origin of the ultraviolet upturn in elliptical galaxies. II. Test of the horizontal branch hypothesis. The Astrophysical Journal, 492, 480.
Yong, H., Demarque, P., & Yi, S. (2000). Mass loss on the horizontal branch: an application to NGC 6791. The Astrophysical Journal, 539, 928.
Acknowledgements
I thank Drs. Philipp Podsiadlowski, Zhanwen Han, and Sukyoung Yi for lending their expertise generously to various parts of research conducted.
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Brown, D. (2018). Some Recent Investigations in Stellar Evolution at the Specola Vaticana. In: Gionti, S. J., G., Kikwaya Eluo, S.J., JB. (eds) The Vatican Observatory, Castel Gandolfo: 80th Anniversary Celebration. Astrophysics and Space Science Proceedings, vol 51. Springer, Cham. https://doi.org/10.1007/978-3-319-67205-2_5
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