New Astronomy

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si47.svg" display="inline" id="d1e5822"><mml:mrow><mml:mi>u</mml:mi><mml:mi>v</mml:mi><mml:mi>b</mml:mi><mml:mi>y</mml:mi><mml:mo linebreak="goodbreak" linebreakstyle="after">−</mml:mo><mml:msub><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:msub><mml:mspace class="nbsp" width="1em"/></mml:mrow></mml:math> Photoelectric photometry of 65 A/F-type candidate stars in the Kepler field: Observations, stellar parameters and variability analysis

A study on the formation of field, binary or multiple stars: A 3D approach through dynamical system

Lightcurves of stars in the Chamaeleon I association

Universal relationships for neutron stars from perturbative approach

Matter power spectrum in a power-law <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si7.svg" display="inline" id="d1e1091"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>G</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity

Diagnozing star formation in the Chamaeleon–Musca dark cloud complex