Results 151 to 160 of about 169 (167)

TED1 Promotes the Assembly of SCFD3‐D14‐D53 to Reinforce Strigolactone Signaling in Rice

Advanced Science, EarlyView.
This study identifies TED1 as a positive regulator of strigolactones (SL) signaling in rice. The ted1 mutants display dwarfism and increased tillering with significantly reduced SLs sensitivity. Through its longer C‐terminal region, TED1 interacts with D53 and D14 to promote the assembly of SCFD3‐D14‐D53, thereby facilitating the efficient ...
Sheng Luo, Chuanyin Wu, Miao Feng, Wenfan Luo, Rong Miao, Jinsheng Qian, Fan Wang, Chunlei Zhou, Bojuan Liu, Jiale Shao, Ziqi Xun, Yehui Xiong, Zhichao Zhao, Cailin Lei, Shanshan Zhu, Yulong Ren, Xin Wang, Xiuping Guo, Haiyang Wang, Zichao Li, Zhijun Cheng, Qibing Lin, Jianmin Wan   +22 more
wiley   +1 more source

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Luminosity and Mass Functions for Low Main-Sequence Stars

Astrophysics and Space Science, 1972
The luminosity function derived for main sequence stars in the neighbourhood of the Sun shows evidence for a flattening in the interval 5≲M v ≲8. An interpretation of this feature by means of theoretical models enables us to deduce the mass function for stars belonging to the main sequence.
exaly   +2 more sources

Luminosity Functions and Mass Functions for Massive Stars: Associations in the Large and Small Magellanic Clouds

1992
UBV CCD photometry has been obtained for 14 OB associations in the Large and Small Magellanic Clouds. The data have been used to construct color-magnitude diagrams for the purpose of investigating the massive-star content of these extragalactic associations.
Robert Hill, Barry F. Madore, Wendy L. Freedman   +2 more
openaire   +1 more source

The Bolometric Luminosity Function for the Lowest Mass Stars

1992
We present a luminosity function (LF) for the coolest stars in three POSSII fields — extending earlier LFs to much lower masses at higher precision than has been acheived previously.
openaire   +1 more source

Luminosity recipes for Solar-type stars as a function of mass, rotation, metallicity and age

We present new comprehensive outputs for models that track luminosity evolution for low-mass stars from 0.5 to 1.2 MSUN over a range of metallicities: Z = (0.006) 0.01 to 0.04. Our calculations use the MESA advanced, open-source 1D stellar evolution code (Paxton et al., 2019; Jermyn et al.
Stephen J. Mojzsis, Lorenzo Roberti, Manuel Scherf, Marco Pignatari   +3 more
openaire   +1 more source

Galaxy and Mass Assembly (GAMA): The Dependence of the Galaxy Luminosity Function on Environment, Redshift and Colour

Monthly Notices of the Royal Astronomical Society, 2014
Jon Loveday, Joss Bland-Hawthorn, Jose Antonio Vazquez-Mata   +2 more
exaly  

Luminosity Function of the Stars and the Problem of the “Missing Mass” in the Solar Neighbourhood

1975
openaire   +1 more source

Galaxy and Mass Assembly (GAMA): Maximum-Likelihood Determination of the Luminosity Function and Its Evolution

Monthly Notices of the Royal Astronomical Society, 2015
Jon Loveday, Steven Phillipps, Joss Bland-Hawthorn   +2 more
exaly  

The Buildup of Stellar Mass and the 3.6 μm Luminosity Function in Clusters From z = 1.25 to z = 0.2

Astronomy and Astrophysics, 2006
Stefano Andreon
exaly  

On the Nature of the Break in the X-Ray Luminosity Function of Low-Mass X-Ray Binaries

Astronomy and Astrophysics, 2011
Konstantin Postnov, M Revnivtsev
exaly