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DOI | 10.1093/pasj/psab112 |
Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate | |
Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro | |
通讯作者 | Teng, HY (corresponding author),Tokyo Inst Technol, Sch Sci, Dept Earth & Planetary Sci, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528551, Japan. |
来源期刊 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
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ISSN | 0004-6264 |
EISSN | 2053-051X |
出版年 | 2022 |
卷号 | 74期号:1 |
英文摘要 | We report the detection of radial velocity (RV) variations in nine evolved G- and K-type giant stars. The observations were conducted at Okayama Astrophysical Observatory. Planets or planet candidates can best explain these regular variations. However, a coincidence of near 280d variability among five of them prevents us from fully ruling out stellar origins for some of the variations, since all nine stars behave similarly in stellar properties. In the planet hypotheses for the RV variations, the planets (including one candidate) may survive close to the boundary of the so-called planet desert around evolved stars, having orbital periods between 255 and 555 d. Besides, they are the least-massive giant planets detected around G- and K-type giant stars, with minimum masses between 0.45 M-J and 1.34 M-J. We further investigated other hypotheses for our detection, yet none of them can better explain regular RV variation. With our detection, we can be convinced that year-long regular variation with amplitude down to 15 m s(-1) for G- and K-type giant stars is detectable. Moreover, we performed simulations to further confirm the detectability of planets around these stars. Finally, we explored giant planets around intermediate-mass stars, and likewise found a four-Jupiter-mass gap (e.g., Santos et al. 2017, A&A, 603, A30), which is probably a boundary of the giant planet population. |
英文关键词 | planetary systems stars: individual (HD 360, epsilon Piscium, HD 10975, HD 79181, HD 99283, nu Leo, HD 161178, HD 219139, gamma Piscium) techniques: radial velocities |
类型 | Article |
语种 | 英语 |
开放获取类型 | Green Submitted |
收录类别 | SCI-E |
WOS记录号 | WOS:000753117100008 |
WOS关键词 | SUBSTELLAR-MASS COMPANIONS ; LONG SECONDARY PERIODS ; STELLAR PARAMETERS ; RED GIANTS ; OSCILLATIONS ; VARIABILITY ; SEARCH ; PERTURBATIONS ; ABUNDANCES ; ACCRETION |
WOS类目 | Astronomy & Astrophysics |
WOS研究方向 | Astronomy & Astrophysics |
资源类型 | 期刊论文 |
条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/376883 |
作者单位 | [Teng, Huan-Yu; Sato, Bun'ei] Tokyo Inst Technol, Sch Sci, Dept Earth & Planetary Sci, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528551, Japan; [Takarada, Takuya; Omiya, Masashi] Natl Inst Nat Sci, Astrobiol Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; [Omiya, Masashi; Ando, Hiroyasu] Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; [Harakawa, Hiroki; Kambe, Eiji; Yoshida, Michitoshi] Natl Inst Nat Sci, Subaru Telescope, Natl Astron Observ Japan, 650 N Aohoku Pl, Hilo, HI 96720 USA; [Izumiura, Hideyuki] Natl Inst Nat Sci, Natl Astron Observ Japan, Okayama Branch Off, Subaru Telescope, Asakuchi, Okayama 7190232, Japan; [Takeda, Yoichi] Naka Ku, 11-2 Enomachi, Hiroshima, Hiroshima 7300851, Japan; [Itoh, Yoichi] Univ Hyogo, Ctr Astron, Nishi Harima Astron Observ, 407-2 Nishigaichi, Sayo, Hyogo 6795313, Japan; [Kokubo, Eiichiro] Grad Univ Adv Studies SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan |
推荐引用方式 GB/T 7714 | Teng, Huan-Yu,Sato, Bun'ei,Takarada, Takuya,et al. Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate[J],2022,74(1). |
APA | Teng, Huan-Yu.,Sato, Bun'ei.,Takarada, Takuya.,Omiya, Masashi.,Harakawa, Hiroki.,...&Kokubo, Eiichiro.(2022).Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,74(1). |
MLA | Teng, Huan-Yu,et al."Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 74.1(2022). |
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