The scientist’s investigation covers issues in Astrophysics, Supernova, Astronomy, Light curve and Galaxy. Her Astrophysics research includes elements of Spectroscopy and Spectral line. Her Supernova research includes themes of Cosmology, Metallicity and White dwarf.
Her research in Light curve intersects with topics in Gamma-ray burst and Pair-instability supernova. When carried out as part of a general Galaxy research project, her work on Extinction, Redshift, Star formation and Interstellar medium is frequently linked to work in Type, therefore connecting diverse disciplines of study. Her Stars study integrates concerns from other disciplines, such as Flare and Tidal disruption event.
Astrophysics, Supernova, Astronomy, Stars and Light curve are her primary areas of study. Her Astrophysics study combines topics from a wide range of disciplines, such as Spectroscopy and Spectral line. Her work carried out in the field of Supernova brings together such families of science as Redshift and Emission spectrum.
Her Light curve research is multidisciplinary, incorporating elements of Absolute magnitude, Metallicity, White dwarf and Near-infrared spectroscopy. Her work in Photometry tackles topics such as Telescope which are related to areas like Observatory. Nidia Morrell interconnects Binary system and Open cluster in the investigation of issues within Radial velocity.
Nidia Morrell mainly focuses on Astrophysics, Supernova, Light curve, Spectral line and Stars. Her Emission spectrum research extends to Astrophysics, which is thematically connected. Her Supernova research is multidisciplinary, relying on both Extinction, Wavelength, Near-infrared spectroscopy and Photometry.
Her Light curve research incorporates elements of Absolute magnitude, Type II supernova, Observatory and Photometric system. Her work focuses on many connections between Stars and other disciplines, such as Star, that overlap with her field of interest in Spectral energy distribution, Be star, Small Magellanic Cloud and Stellar evolution. The various areas that Nidia Morrell examines in her Galaxy study include Dipolar field, Brightness, Stellar classification and Sample.
Her primary scientific interests are in Astrophysics, Supernova, Stars, Light curve and Spectral line. In her research, Nidia Morrell performs multidisciplinary study on Astrophysics and Type. The study incorporates disciplines such as Wavelength, Near-infrared spectroscopy, Extinction, Luminosity and Photometry in addition to Supernova.
Nidia Morrell has researched Luminosity in several fields, including Telescope and Observatory. In general Stars, her work in Red supergiant, Globular cluster and Orbital eccentricity is often linked to Diagram linking many areas of study. Her research in Emission spectrum intersects with topics in Ejecta and Redshift.
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.
THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617
B. J. Shappee;J. L. Prieto;D. Grupe;C. S. Kochanek.
The Astrophysical Journal (2014)
SB9: The Ninth Catalogue of Spectroscopic Binary Orbits
D. Pourbaix;A. A. Tokovinin;A. H. Batten;F. C. Fekel.
arXiv: Astrophysics (2004)
S B 9 : The ninth catalogue of spectroscopic binary orbits
Dimitri Pourbaix;Dimitri Pourbaix;Andrei A. Tokovinin;Alen H. Batten;Francis C. Fekel.
Astronomy and Astrophysics (2004)
The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars
Helmut A. Abt;Nidia I. Morrell.
Astrophysical Journal Supplement Series (1995)
Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
M. R. Drout;A. L. Piro;B. J. Shappee;C. D. Kilpatrick.
Science (2017)
The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae
Carlos Contreras;Mario Hamuy;M. M. Phillips;Gaston Folatelli.
arXiv: Cosmology and Nongalactic Astrophysics (2009)
An asymptotic-giant-branch star in the progenitor system of a type Ia supernova.
Mario Hamuy;M. M. Phillips;Nicholas B. Suntzeff;José Maza.
Nature (2003)
The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae
Gastón Folatelli;Gastón Folatelli;M. M. Phillips;Christopher R. Burns;Carlos Contreras.
The Astronomical Journal (2010)
Characterizing the V-band light-curves of hydrogen-rich type II supernovae
Joseph P. Anderson;Santiago González-Gaitán;Mario Hamuy;Claudia P. Gutiérrez.
arXiv: High Energy Astrophysical Phenomena (2014)
The Galactic O-Star Spectroscopic Survey. I. Classification System and Bright Northern Stars in the Blue-Violet at R~2500
A. Sota;J. Maiz Apellaniz;Nolan R. Walborn;Emilio J. Alfaro.
Astrophysical Journal Supplement Series (2011)
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