编译 | 李言
Science,迷信 18 AUG 2023, Volume 381 Issue 6659
《迷信》2022年8月18日,第381卷,出书6659期
?周论
生物物理学Biophysics
Alcanivorax borkumensis biofilms enhance oil degradation by interfacial tubulation
泊库岛食烷菌生物膜经由界面管化增长煤油降解
▲ 作者:M. PRASAD, N. OBANA et al.
▲ 链接:https://www.science.org/doi/full/10.1126/science.adf3345
▲ 摘要:
在破费烷烃的历程中 ,泊库岛食烷菌会在油滴周围组成生物膜,文导但这在降解历程中所起的迷信熏染尚不清晰 。
咱们发现了生物膜形态的出书变更取决于对于煤油破费的顺应 :持久的吐露导致树突状生物膜的泛起,经由界面的周论管状影响优化了煤油破费 。原位微流体跟踪使咱们可能将管状与界面细胞有序中的文导部份缺陷分割起来。
咱们演示了经由运用限度来定位缺陷来操作液滴变形,迷信从而使患上液滴发生突出 。出书咱们开拓了一个模子来声名生物膜形态,周论将微管化与界面张力飞腾以及细胞疏水性削减分割起来。文导
▲ Abstract:
During the consumption of alkanes,迷信 Alcanivorax borkumensis will form a biofilm around an oil droplet, but the role this plays during degradation remains unclear. We identified a shift in biofilm morphology that depends on adaptation to oil consumption: Longer exposure leads to the appearance of dendritic biofilms optimized for oil consumption effected through tubulation of the interface. In situ microfluidic tracking enabled us to correlate tubulation to localized defects in the interfacial cell ordering. We demonstrate control over droplet deformation by using confinement to position defects, inducing dimpling in the droplets. We developed a model that elucidates biofilm morphology, linking tubulation to decreased interfacial tension and increased cell hydrophobicity.
天体物理学Astrophysics
A massive helium star with a sufficiently strong magnetic field to form a magnetar
有饶富强磁场组成磁星的大品质氦恒星
▲ 作者:TOMER SHENAR, GREGG A. WADE, PABLO MARCHANT et al.
▲ 链接:https://www.science.org/doi/full/10.1126/science.ade3293
▲ 摘要:
磁星是高度磁化的中子星,但组成机制尚不清晰 。出书光谱以发射线为主的周论富氦恒星 ,被称为沃尔夫-拉叶星。
咱们用光谱偏振法审核了双星零星HD 45166,并运用档案数据重新合成了它的轨道。咱们发现该星系中有一颗沃尔夫-拉叶星,其品质是太阳的2倍 ,磁场为43千高斯。
恒星演化合计表明 ,这颗星将爆炸成为一颗超新星,而它的磁场强盛到足以让超新星留下磁星遗迹。咱们提出磁化的沃尔夫-拉叶星是由两颗低品质氦恒星并吞组成的。
▲ Abstract :
Magnetars are highly magnetized neutron stars, the formation mechanism of which is unknown. Hot helium-rich stars with spectra dominated by emission lines are known as Wolf-Rayet stars. We observed the binary system HD 45166 using spectropolarimetry and reanalyzed its orbit using archival data. We found that the system contains a Wolf-Rayet star with a mass of 2 solar masses and a magnetic field of 43 kilogauss. Stellar evolution calculations indicate that this component will explode as a supernova, and that its magnetic field is strong enough for the supernova to leave a magnetar remnant. We propose that the magnetized Wolf-Rayet star formed by the merger of two lower-mass helium stars.
光学Optics
Overcoming losses in superlenses with synthetic waves of complex frequency
用复频率分解波克制超透镜斲丧
▲ 作者 :FUXIN GUAN, XIANGDONG GUO, KEBO ZENG et al.
▲ 链接:https://www.science.org/doi/full/10.1126/science.adi1267
▲ 摘要:
揭示出光阴衰减行动的复频率光波被提出经由引入伪造增益来对于消超透镜的本征损失