His primary areas of study are Astrophysics, Astronomy, Stars, Galaxy and Metallicity. His Exoplanet, Spectrograph, Star formation and Spectral line study in the realm of Astronomy interacts with subjects such as Espresso. Paolo Molaro has researched Stars in several fields, including Halo and Galactic halo.
His Milky Way, Abundance of the chemical elements and Galaxy formation and evolution study, which is part of a larger body of work in Galaxy, is frequently linked to Context, bridging the gap between disciplines. His Metallicity study combines topics from a wide range of disciplines, such as Stellar mass loss, Equivalent width, Supernova and Photometry. The various areas that Paolo Molaro examines in his Nucleosynthesis study include Subgiant, Standard Model and Physics beyond the Standard Model.
The scientist’s investigation covers issues in Astrophysics, Stars, Astronomy, Spectral line and Metallicity. His study in Galaxy, Redshift, Quasar, Galactic halo and Radial velocity is carried out as part of his Astrophysics studies. His work in the fields of Galaxy, such as Milky Way, intersects with other areas such as Context and Population.
In his research, Deuterium is intimately related to Lithium, which falls under the overarching field of Stars. His Spectral line study incorporates themes from Line, Absorption, Ionization, Nova and Interstellar medium. The Metallicity study combines topics in areas such as K-type main-sequence star, s-process, Spiral galaxy and Photometry.
Paolo Molaro mainly focuses on Astrophysics, Stars, Astronomy, Planet and Radial velocity. His Astrophysics study frequently draws connections between related disciplines such as Spectral line. His study in Stars is interdisciplinary in nature, drawing from both Galaxy and Lithium.
In general Astronomy study, his work on Nucleosynthesis and Imaging spectroscopy often relates to the realm of X-ray fluorescence and Portrait, thereby connecting several areas of interest. Paolo Molaro works mostly in the field of Planet, limiting it down to topics relating to Accretion and, in certain cases, Stellar atmosphere and Deuterium, as a part of the same area of interest. His Metallicity study combines topics in areas such as Star formation and Supernova.
His primary scientific interests are in Astrophysics, Exoplanet, Stars, Astronomy and Spectrograph. His Astrophysics research is multidisciplinary, relying on both Spectral line and Absorption. His studies deal with areas such as Planetary system, Spectroscopy, Radial velocity and Atmospheric chemistry as well as Exoplanet.
Paolo Molaro specializes in Stars, namely Big Bang nucleosynthesis. His research on Spectrograph also deals with topics like
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Review of Particle Physics
K. A. Olive;K. Agashe;C. Amsler;M. Antonelli.
Chinese Physics C (2014)
APS : Review of Particle Physics, 2018-2019
M Tanabashi;P Richardson;A Bettini;A Vogt.
Physical Review D (2018)
Big-Bang Nucleosynthesis
Brian D. Fields;Paolo Molaro;Subir Sarkar.
arXiv: Cosmology and Nongalactic Astrophysics (2014)
Oxford University Press : Review of Particle Physics, 2020-2021
P A Zyla;P Richardson;O Zenin;A Bettini.
PTEP (2020)
First stars V - abundance patterns from C to Zn and supernova yields in the early galaxy
R. Cayrel;E. Depagne;M. Spite;V. Hill.
Astronomy and Astrophysics (2004)
The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters
R. G. Gratton;P. Bonifacio;A. Bragaglia;E. Carretta.
Astronomy and Astrophysics (2001)
First stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements
M. Spite;R. Cayrel;B. Plez;V. Hill.
arXiv: Astrophysics (2004)
The metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities and lithium abundances
L. Sbordone;P. Bonifacio;E. Caffau;H.-G. Ludwig.
arXiv: Astrophysics of Galaxies (2010)
Measurement of stellar age from uranium decay.
R. Cayrel;V. Hill;T. C. Beers;B. Barbuy.
Nature (2001)
The metal-poor end of the Spite plateau - I. Stellar parameters, metallicities, and lithium abundances
L. Sbordone;P. Bonifacio;P. Bonifacio;E. Caffau;H. G. Ludwig;H. G. Ludwig.
Astronomy and Astrophysics (2010)
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