PSR B0329+54:半径9.62km,质量1.44Msun,原质量14Msun,光谱B0V。, 视频播放量 3249、弹幕量 9、点赞数 61、投硬币枚数 7、收藏人数 48、转发人数 3, 视频作者 HD10180-C, 作者简介 恭喜你发现了一个宝藏up……,相关视频:参宿五—B型恒星的历史与未来,恰好可以变中子星
PSR (B0329+54) CNS Rmx $1.49 Artisti: TON 618 Remixers: CNS Lunghezza:5:39 Pubblicato:2024-04-26 BPM:140 Chiave:E Major Genere:Techno (Peak Time / Driving) Etichetta: Exodus Recordings Brani consigliati Titolo / Artisti Etichetta / Remixer Genere / BPM & Chiave Pubblicato 1 SMA...
冲星PSR B0329+54在408 MHz 、610 MHz 、925 MHz 、1408 MHz 、1642 MHz 5个不同频率下的累积脉冲 轮廓进行了高斯拟合研究;并对脉冲星辐射区不同成份的频谱特性进行分析.因为所用的频率范围比较 宽、而且这5个频段上PSR B0329+54的累积脉冲轮廓的信噪比是比其它脉冲星的都高、因此该脉冲星是 应用成份分解...
Psr B0329+54 短评 下载豆瓣客户端 豆瓣6.0全新发布× 豆瓣 扫码直接下载 iPhone·Android >Psr B0329+54 作者:Aloysius, Dewayne Rocky 页数:136 isbn:6139126762 书名:Psr B0329+54
We have investigated the mode changing properties of PSR B0329+54 using 31 epochs of simultaneous 13 cm/3 cm single-pulse observations obtained with the Shanghai Tian Ma 65 m telescope. The pulsar was found in the abnormal emission mode 17 times, accounting for simi...
B0329 + 54的模式改变特性。在异常发射模式下发现脉冲星17次,占总观察时间41.6小时的〜13%。单脉冲分析表明,模式变化在几个旋转周期内以13 cm / 3 cm同时发生。我们检测到偶发的明亮和狭窄脉冲,其峰值通量密度比两个频带中的积分曲线都高10倍。在3 cm处,正常模式和异常模式下的单个脉冲分别亮约0.66%和...
The stability of the integrated profile of PSR B0329 + 54 at 1,540 MHz is studied with the observation data of the Nanshan 25-m radio telescope of up to 45... HZX Chen - 《Astronomische Nachrichten A Journal on All Fields of Astronomy》 被引量: 0发表: 2021年 加载更多站...
Track PSR (B0329+54) CNS Rmx $1.49 Artists: TON 618 Remixers: CNS Length:5:39 Released:2024-09-11 BPM:140 Key:E Major Genre:Techno (Peak Time / Driving) Label: LW Recordings Recommended Tracks Title / Artists Label / Remixers Genre / BPM & Key Released 1 Incross The Glow ...
PSR (B0329+54) CNS Rmx $1.49 Artistes: TON 618 Remixers: CNS Durée:5:39 Sorties:2024-04-26 BPM:140 Clé:E Major Genre:Techno (Peak Time / Driving) Label: Exodus Recordings Pistes recommandées Titre / Artistes Label / Remixers Genre / BPM & Clé Sorties 1 SMACKIN Original ...
A periodicity in the radio frequency spectrum of PSR 0329 + 54 has been reported by Sturrock et al. Approximately 12 times the data available to them were analysed, with no sign of any obvious, consistent periodicity. It is concluded that the apparent periodicity is due to random scintillatio...