Zobrazeno 1 - 10
of 38
pro vyhledávání: '"Sanemichi Z. Takahashi"'
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 1, p 60 (2023)
Secular gravitational instability (GI) is one promising mechanism for explaining planetesimal formation. Previous studies of secular GI utilized a razor-thin disk model and derived the growth condition in terms of vertically integrated physical value
Externí odkaz:
https://doaj.org/article/e1e76141dea145ce9f6a90a8acf5f7fa
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 2, p 120 (2023)
We investigate the gravitational instability (GI) of dust ring structures and the formation of planetesimals by their gravitational collapse. The normalized dispersion relation of a self-gravitating ring structure includes two parameters that are rel
Externí odkaz:
https://doaj.org/article/221af9e10a6e43a78a16f5b0dca5deab
We investigate the gravitational instability (GI) of dust-ring structures and the formation of planetesimals by their gravitational collapse. The normalized dispersion relation of a self-gravitating ring structure includes two parameters that are rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c215285f752c9a6f4deeb72277c0d25
http://arxiv.org/abs/2211.02311
http://arxiv.org/abs/2211.02311
Autor:
Takayuki Muto, Yasuhiro Hasegawa, Tomohiro Ono, Kengo Tomida, Hauyu Baobab Liu, Takashi Tsukagoshi, Hideko Nomura, Mihoko Konishi, Sanemichi Z. Takahashi, Ruobing Dong, Jun Hashimoto, Akimasa Kataoka, Michihiro Takami, Kazuhiro D. Kanagawa, Munetake Momose, Michael L. Sitko
We present Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations of dust continuum emission of the disk around WW Cha. The dust continuum image shows a smooth disk structure with a faint (low-contrast) dust ring, extending from $\si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f006596a4eea985e67aa6d2bfa7fb64
Secular gravitational instability (GI) is one of the promising mechanisms for creating annular substructures and planetesimals in protoplanetary disks. We perform numerical simulations of the secular GI in a radially extended disk with inward driftin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::67d388a3eeeb3f50ed4b9b477499f004
http://arxiv.org/abs/2008.02564
http://arxiv.org/abs/2008.02564
Autor:
Kengo Tomida, Sanemichi Z. Takahashi, Takashi Tsukagoshi, Jiaqing Bi, Tomohiro Ono, Michihiro Takami, Jun Hashimoto, Mihoko Konishi, Takayuki Muto, Yasuhiro Hasegawa, Kazuhiro D. Kanagawa, Munetake Momose, Hideko Nomura, Hauyu Baobab Liu, Akimasa Kataoka, Rebecca G. Martin, Nienke van der Marel, Jeremy L. Smallwood, Ruobing Dong, Michael L. Sitko
GW Ori is a hierarchical triple system which has a rare circumtriple disk. We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of 1.3 mm dust continuum and 12CO J=2-1 molecular gas emission of the disk. For the first time, we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4ed4ae0d00e6e678e804fe7d6e0dc1f
http://arxiv.org/abs/2004.03135
http://arxiv.org/abs/2004.03135
Autor:
Takashi Tsukagoshi, Hideko Nomura, Takayuki Muto, Ryohei Kawabe, Kazuhiro D. Kanagawa, Satoshi Okuzumi, Shigeru Ida, Catherine Walsh, Tom J. Millar, Sanemichi Z. Takahashi, Jun Hashimoto, Taichi Uyama, Motohide Tamura
Publikováno v:
Tsukagoshi, T, Nomura, H, Muto, T, Kawabe, R, Kanagawa, K D, Okuzumi, S, Ida, S, Walsh, C, Millar, T J, Takahashi, S Z, Hashimoto, J, Uyama, T & Tamura, M 2022, ' ALMA high-resolution multiband analysis for the protoplanetary disk around TW Hya ', The Astrophysical Journal, vol. 928, no. 1, 49 . https://doi.org/10.3847/1538-4357/ac5111
We present a high-resolution (2.5 au) multiband analysis of the protoplanetary disk around TW Hya using ALMA long baseline data at Bands 3, 4, 6, and 7. We aim to reconstruct a high-sensitivity millimeter continuum image and revisit the spectral inde
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 472:532-541
We consider whether the maximum mass of first stars is imposed by the protostellar spin, i.e., by the so-called $\Omega\Gamma$-limit, which requires the sum of the radiation and centrifugal forces at the stellar surface be smaller than the inward pul
Autor:
Tom J. Millar, Satoshi Okuzumi, Hideko Nomura, Motohide Tamura, Sanemichi Z. Takahashi, Ryohei Kawabe, Takayuki Muto, Taichi Uyama, Takashi Tsukagoshi, Jun Hashimoto, Catherine Walsh, Kazuhiro D. Kanagawa, Shigeru Ida
Publikováno v:
Tsukagoshi, T, Muto, T, Nomura, H, Kawabe, R, Kanagawa, K D, Okuzumi, S, Ida, S, Walsh, C, Millar, T J, Takahashi, S Z, Hashimoto, J, Uyama, T & Tamara, M 2019, ' Discovery of an au-scale Excess in Millimeter Emission from the Protoplanetary Disk around TW Hya ', The Astrophysical Journal Letters, vol. 878, no. 1, L8 . https://doi.org/10.3847/2041-8213/ab224c
We report the detection of an excess in dust continuum emission at 233~GHz (1.3~mm in wavelength) in the protoplanetary disk around TW~Hya revealed through high-sensitivity observations at $\sim$3~au resolution with the Atacama Large Millimeter/submi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f14d1cb34ea914d0b064cfcacb231cd
https://eprints.whiterose.ac.uk/147059/1/Tsukagoshi_2019_ApJL_878_L8.pdf
https://eprints.whiterose.ac.uk/147059/1/Tsukagoshi_2019_ApJL_878_L8.pdf
Autor:
Kazuhiro D. Kanagawa, Kengo Tomida, Hideko Nomura, Yasuhiro Hasegawa, Takashi Tsukagoshi, Seongjoong Kim, Jun Hashimoto, Takayuki Muto, Akimasa Kataoka, Hauyu Baobab Liu, Sanemichi Z. Takahashi, Ruobing Dong, Seokho Lee, Mihoko Konishi, Michael L. Sitko, Munetake Momose
We observe the dust continuum at 225 GHz and CO isotopologue (12CO, 13CO, and C18O) J=2-1 emission lines toward the CR Cha protoplanetary disk using the Atacama Large Millimeter/Submillimeter Array (ALMA). The dust continuum image shows a dust gap-ri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f8eb7fae2c69d617a6499e12c06fd38