招待 发表于 2025-3-28 14:36:33
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu平息 发表于 2025-3-28 22:14:22
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu向下 发表于 2025-3-29 01:04:31
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same cataloguWordlist 发表于 2025-3-29 06:35:30
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu刚开始 发表于 2025-3-29 10:13:47
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same cataloguAtrium 发表于 2025-3-29 13:58:53
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same cataloguAcupressure 发表于 2025-3-29 18:23:50
http://reply.papertrans.cn/83/8254/825347/825347_47.png装饰 发表于 2025-3-29 21:38:12
http://reply.papertrans.cn/83/8254/825347/825347_48.pngOutspoken 发表于 2025-3-30 03:34:50
http://reply.papertrans.cn/83/8254/825347/825347_49.pnglimber 发表于 2025-3-30 05:24:51
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.th updated values for their distances, proper motions and radial velocities (Gliese & Jahreiss 1991) space velocity dispersions are calculated for these stars. It is found that the total velocity dispersion of the flare stars (σ=30±3 km s.) is similar to that of the F5 V stars from the same catalogu