Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-25T18:19:55.608Z Has data issue: false hasContentIssue false
  • English
  • Français

Implication of the period-magnitude relation for massive AGB stars and its astronomical applications

Published online by Cambridge University Press:  06 February 2024

Akiharu Nakagawa Open the ORCID record for Akiharu Nakagawa [Opens in a new window] ,
Tomoharu Kurayama ,
Hiroshi Sudou  and
Gabor Orosz Open the ORCID record for Gabor Orosz [Opens in a new window]
Akiharu Nakagawa*
Affiliation:
Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065, Japan
Tomoharu Kurayama
Affiliation:
Teikyo University of Science, 2-2-1 Senju-Sakuragi, Adachi-ku, Tokyo 120-0045, Japan
Hiroshi Sudou
Affiliation:
Department of General Engineering, National Institute of Technology, Sendai College, Natori Campus, 48 Nodayama, Medeshima-Shiote, Natori-shi, Miyagi 981-1239, Japan
Gabor Orosz
Affiliation:
Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, Netherlands
*
email: nakagawa@sci.kagoshima-u.ac.jp
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present astrometric very long baseline interferometry (VLBI) studies of AGB stars. To understand the properties and evolution of AGB stars, distances are an important parameter. The distribution and kinematics of their circumstellar matter are also revealed with the VLBI method. We used the VERA array to observe 22 GHz H2O masers in various subclasses of AGB stars. Parallaxes of the three OH/IR stars NSV17351, OH39.7+1.5, IRC−30363, and the Mira-type variable star AW Tau were newly obtained. We present the circumstellar distribution and kinematics of H2O masers around NSV17351. The absolute magnitudes in mid-infrared bands of OH/IR stars with very long pulsation periods were investigated and a period-magnitude relation in the WISE W3 band, MW3 = (−7.21 ± 1.18) log P + (9.25 ± 3.09), was found for the Galactic AGB stars. The VLBI is still a powerful tool for parallax measurements of the Galactic AGB stars surrounded by thick dust shells.

Keywords

VLBIAstrometryMasersAGB starsOH/IR stars
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S376: At the crossroads of astrophysics and cosmology: Period–luminosity relations in the 2020s , December 2022 , pp. 159 - 179
Check for updates
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Asaki, Y., Deguchi, S., Imai, H., et al. 2010, ApJ, 721, 267 Google Scholar
Baba, J., Saitoh, T. R., & Wada, K. 2013, ApJ, 763, 46 Google Scholar
Baba, J. 2015, MNRAS, 454, 2954 Google Scholar
Burns, R. A., Handa, T., Nagayama, T., et al. 2016, MNRAS, 460, 283 Google Scholar
Chiavassa, A., Freytag, B., & Schultheis, M. 2018, A&A, 617, L1 Google Scholar
Chibueze, J. O., Omodaka, T., Urago, R., et al. 2019, PASJ, 71, 92 Google Scholar
Choi, Y. K., Hirota, T., Honma, M., et al. 2008, PASJ, 60, 1007 Google Scholar
Cox, J. P. 1980, Theory of Stellar Pulsation (Princeton: Princeton University Press)Google Scholar
Engels, D., Etoka, S., Gérard, E., et al. 2015, in: Kerschbaum, F., Wing, R. F., & Hron, J. (eds.), Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time, ASP Conf. Ser., 497, p. 473Google Scholar
Etoka, S., Engels, D., Gérard, E., et al. 2018, in: Tarchi, A., Reid, M. J., Castangia, & P. (eds.), Astrophysical Masers: Unlocking the Mysteries of the Universe, Proc. IAU Symp. No. 336 (Cambridge: Cambridge University Press), p. 381Google Scholar
Feast, M. W. 2009, in: Ueta, T., Matsunaga, N., & Ita, Y.. (eds.), AGB Stars and Related Phenomena (Tokyo: NAOJ), p. 48Google Scholar
Fomalont, E. 1981, NRAO Newsletter, 3, 3 Google Scholar
Collaboration, Gaia, Vallenari, A., Brown, A. G. A., et al. 2023, A&A, 674, A1 Google Scholar
Goldman, S. R., van Loon, J. T., Zijlstra, A. A., et al. 2017, MNRAS, 465, 403 Google Scholar
Habing, H. J. 1996, A&AR, 7, 97 Google Scholar
Höfner, S. & Olofsson, H. 2018, A&AR, 26, 1 Google Scholar
Honma, M., Kijima, M., Suda, H., et al. 2008, PASJ, 60, 935 Google Scholar
Imai, H., Sakai, N., Nakanishi, H., et al. 2012, PASJ, 64, 142 Google Scholar
Ita, Y., Tanabé, T., Matsunaga, N., et al. 2004, MNRAS, 347, 720 Google Scholar
Justtanont, K., Barlow, M. J., Blommaert, J., et al. 2015, A&A, 578, A115 Google Scholar
Kamezaki, T., Nakagawa, A., Omodaka, T., et al. 2012, PASJ, 64, 7 Google Scholar
Kamezaki, T., Kurayama, T., Nakagawa, A., et al. 2014, PASJ, 66, 107 Google Scholar
Kamezaki, T., Nakagawa, A., Omodaka, T., et al. 2016, PASJ, 68, 71 Google Scholar
Kamezaki, T., Nakagawa, A., Omodaka, T., et al. 2016, PASJ, 68, 75 Google Scholar
Kamizuka, T., Nakada, Y., Yanagisawa, K., et al. 2020, ApJ, 897, 42 Google Scholar
Kamohara, R., Bujarrabal, V., Honma, M., et al. 2010, A&A, 510, A69 Google Scholar
Karakas, A. I. & Lattanzio, J. C. 2014, PASA, 31, e030 CrossRefGoogle Scholar
Karambelkar, V. R., Adams, S. M., Whitelock, P. A., et al. 2019, ApJ, 877, 110 Google Scholar
Kawaguchi, N., Sasao, T., & Manabe, S. 2000, Proc. SPIE, 4015, 544 Google Scholar
Kemper, F., de Koter, A., Waters, L. B. F. M., et al. 2002, A&A, 384, 585 Google Scholar
Kurayama, T., Sasao, T., & Kobayashi, H. 2005, ApJ, 627, L49 Google Scholar
Kusuno, K., Asaki, Y., Imai, H., & Oyama, T. 2013, ApJ, 774, 107 Google Scholar
Le Squeren, A. M., Baudry, A., Brillet, J., & Darchy, B. 1979, A&A, 72, 39 Google Scholar
Lin, C. C., & Shu, F. H. 1964, ApJ, 140, 646 Google Scholar
te Lintel Hekkert, P., Caswell, J. L., Habing, H. J., et al. 1991, A&AS, 90, 327Google Scholar
Matsuno, M., Nakagawa, A., Morita, A., et al. 2020, PASJ, 72, 56 Google Scholar
Min, C., Matsumoto, N., Kim, M. K., et al. 2014, PASJ, 66, 38 Google Scholar
Motogi, K., Sorai, K., Honma, M., et al. 2016, PASJ, 68, 69 Google Scholar
Nakagawa, A., Tsushima, M., Ando, K., et al. 2008, PASJ, 60, 1013 Google Scholar
Nakagawa, A., Omodaka, T., Handa, T., et al. 2014, PASJ, 66, 101 Google Scholar
Nakagawa, A., Kurayama, T., Matsui, M., et al. 2016, PASJ, 68, 78 Google Scholar
Nakagawa, A., Kurayama, T., Orosz, G., et al. 2018, in: Tarchi, A., Reid, M. J., & Castangia, P. (eds.), Astrophysical Masers: Unlocking the Mysteries of the Universe, Proc. IAU Symp. No. 336 (Cambridge: Cambridge University Press), p. 365Google Scholar
Nakagawa, A., Kurayama, T., Orosz, G., et al. 2019, in: Kerschbaum, F., Groenewegen, M., & Olofsson, H. (eds.), Why Galaxies Care about AGB Stars: A Continuing Challenge through Cosmic Time, Proc. IAU Symp. No. 343 (Cambridge: Cambridge University Press), p. 476Google Scholar
Nakagawa, A., Morita, A., Sakai, N., et al. 2023, PASJ, 75, 529 Google Scholar
Nakagawa, A., Kurayama, T., Sudou, H., Orosz, G. 2023, This work Google Scholar
Nikzat, F., Ferreira Lopes, C. E., Catelan, M., et al. 2022, A&A, 660, A35 Google Scholar
Nyman, L.-A., Hall, P. J., & Olofsson, H. 1998, A&AS, 127, 185 Google Scholar
Nyu, D., Nakagawa, A., Matsui, M., et al. 2011, PASJ, 63, 63 Google Scholar
Orosz, G., Imai, H., Dodson, R., et al. 2017, AJ, 153, 119 Google Scholar
Oyama, T., Kono, Y., Suzuki, S., et al. 2016, PASJ, 68, 105 Google Scholar
Reid, M. J., Menten, K. M., Brunthaler, A., et al. 2019, ApJ, 885, 131 Google Scholar
Sellwood, J. A., & Carlberg, R. G. 1984, ApJ, 282, 61 Google Scholar
Sparke, L. S., & Gallagher, J. S. 2000, Galaxies in the Universe (Cambridge: Cambridge University Press)Google Scholar
Sudou, H., Omodaka, T., Murakami, K., et al. 2019, PASJ, 71, 16 Google Scholar
Takeuti, M., Nakagawa, A., Kurayama, T., et al. 2013, PASJ, 65, 60 Google Scholar
Thompson, A. R., Moran, J. M., & Swenson, G. W. 2001, Interferometry and Synthesis in Radio Astronomy, 2nd Edition (New York: Wiley)Google Scholar
Urago, R., Yamaguchi, R., Omodaka, T., et al. 2020, PASJ, 72, 57 Google Scholar
Collaboration, VERA, Hirota, T., Nagayama, T., et al. 2020, PASJ, 72, 50 Google Scholar
Vlemmings, W. H. T., van Langevelde, H. J., Diamond, P. J., Habing, H. J., & Schilizzi, R. T. 2003, A&A, 407, 213 Google Scholar
Vlemmings, W. H. T., & van Langevelde, H. J. 2007, A&A, 472, 547 Google Scholar
Vlemmings, W. H. T., Khouri, T., & Tafoya, D. 2021, A&A, 654, A18 Google Scholar
Watson, C. L., Henden, A. A., & Price, A. 2006, in: Warner, B. D., Foote, J., Kenyon, D. A., & Mais, D. (eds.), Symposium on Telescope Science, Proc. 25th Ann. Conf. of the Soc. for Astron. Sci. (Big Bear Lake: SAS), p. 47Google Scholar
Wood, P. R., Alcock, C., Allsman, R. A., et al. 1999, in: Le Bertre, T., Lebre, A., & Waelkens, C. (eds.), Asymptotic Giant Branch Stars, Proc. IAU Symp. No. 191 (San Francisco: ASP), p. 151 Google Scholar
Wright, E. L., Eisenhardt, P. R. M., Mainzer, A. K., et al. 2010, AJ, 140, 1868 Google Scholar
Xu, S., Zhang, B., Reid, M. J., et al. 2018, ApJ, 859, 14 Google Scholar
Zhang, B., Reid, M. J., Menten, K. M., Zheng, X. W., & Brunthaler, A. 2012, A&A, 544, A42 Google Scholar
Zhang, B., Zheng, X., Reid, M. J., et al. 2017, ApJ, 849, 99 CrossRefGoogle Scholar