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OB2-1 protein, human

Known as: OB2-1 transcription factor, human 
National Institutes of Health

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Related topics

2 relations

Broader (2)

DNA-Binding ProteinsTRANSCRIPTION FACTOR

Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2018
2018
Massive, wide binaries as tracers of massive star formation
Massive stars can be found in wide (hundreds to thousands AU) binaries with other massive stars. We use $N$-body simulations to… 
2013
2013
Modeling of atmospheres of the brightest stars belonging to the Cyg OB2 association
We present the results of modeling of the spectrum of the brightest stars belonging to the Cyg OB2 association - #7 (O3If*) and… 
Review
2012
Review
2012
I. A pathfinder
Context. Cygnus X is one of the most complex areas in the sky, rich in massive stars; Cyg OB2 (2600 stars, 120 O stars) and other… 
Review
2009
Review
2009
OB STARS AND STELLAR BOW SHOCKS IN CYGNUS-X: A NOVEL LABORATORY ESTIMATING STELLAR MASS LOSS RATES
We use mid-infrared images from the Spitzer Space Telescope Cygnus X Legacy Survey to search for stellar bow shocks (BSs), a… 
2003
2003
Spectroscopic Analysis of Cyg OB2 Supergiants Using Unified Model Atmospheres
2001
2001
An analysis of HST UV spectra of Cyg OB2 stars
As a first step of a vigorous program to investigate the Wind Momentum - Luminosity Relationship (WLR) of Galactic O-stars by… 
2001
2001
Interstellar C2 and CN toward the Cyg OB2 association A case study of X-ray induced chemistry
An analysis of deep optical echelle spectra towards six stars in the Cyg OB2 (VI Cygni) association is presented. Interstellar… 
1999
1999
Fundamental parameters of galactic luminous OB stars. III. Spectroscopic analysis of O stars in Cygnus OB2
We present the results of the spectral analysis of 11 OB stars in Cyg OB2, among them seven giants and supergiants. The projected… 
1996
1996
OB2 統制した豊富環境で生育したラットの行動特徴II : Hebb-Williams迷路学習(日本動物心理学会第55回大会発表要旨)
1994
1994
VLA observations of Cyg OB2 No. 5: detection of a weak radio companion and new observations and models for the main component.
We present Very Large Array observations of the contact binary star Cyg OB2 No. 5 obtained over the last four years. A weak (∼0.6… 
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