His primary areas of study are Astrophysics, Galaxy, Luminous infrared galaxy, Star formation and Astronomy. Within one scientific family, Aaron S. Evans focuses on topics pertaining to Spectral line under Astrophysics, and may sometimes address concerns connected to Stellar evolution. As part of one scientific family, Aaron S. Evans deals mainly with the area of Galaxy, narrowing it down to issues related to the Line, and often Supernova.
The study incorporates disciplines such as Spectroscopy, Infrared, Vibrational temperature, Observatory and Spitzer Space Telescope in addition to Luminous infrared galaxy. He has included themes like Star cluster, Redshift and Excitation temperature in his Star formation study. His biological study focuses on Interstellar medium.
His primary scientific interests are in Astrophysics, Galaxy, Luminous infrared galaxy, Astronomy and Star formation. Astrophysics is frequently linked to Infrared in his study. His studies in Galaxy integrate themes in fields like Line and Stars.
Aaron S. Evans interconnects Wavelength, Surface brightness, Universe and QSOS in the investigation of issues within Luminous infrared galaxy. The various areas that Aaron S. Evans examines in his Star formation study include Molecular cloud, Spectroscopy, Galaxy formation and evolution, Spiral galaxy and Stellar evolution. His Active galactic nucleus research is multidisciplinary, incorporating perspectives in Equivalent width and Emission spectrum.
Aaron S. Evans spends much of his time researching Astrophysics, Galaxy, Star formation, Luminous infrared galaxy and Astronomy. Astrophysics and Infrared are commonly linked in his work. His Galaxy study frequently draws connections between related disciplines such as Stars.
He combines subjects such as Extinction, Star cluster, Spatially resolved and Millimeter with his study of Star formation. His Luminous infrared galaxy study integrates concerns from other disciplines, such as Redshift, Very large array, Jansky, Excited state and Submillimeter Array. As a part of the same scientific study, Aaron S. Evans usually deals with the Active galactic nucleus, concentrating on Dust lane and frequently concerns with Atacama Large Millimeter Array.
His scientific interests lie mostly in Astrophysics, Galaxy, Star formation, Luminosity and Luminous infrared galaxy. His Astrophysics research includes elements of Astronomy and Infrared. His study in the field of Hubble space telescope, Spiral galaxy, Luminosity function and Galaxy merger is also linked to topics like Outflow.
His study in Spiral galaxy is interdisciplinary in nature, drawing from both Accretion and Star. His study looks at the relationship between Star formation and topics such as Galaxy formation and evolution, which overlap with Megamaser, Spectral line, Interstellar medium and Starburst region. His Luminosity study which covers Bipolar outflow that intersects with Supernova.
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.
Black hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231
P. P. Van der Werf;K. G. Isaak;R. Meijerink;M. Spaans.
arXiv: Astrophysics of Galaxies (2010)
Molecular Gas in the Z = 2.8 Submillimeter Galaxy SMM 02399-0136
D T Frayer;R J ivison;R J ivison;N Z Scoville;Min S. Yun.
The Astrophysical Journal (1998)
High Resolution Mid-Infrared Imaging of Ultraluminous Infrared Galaxies*
B. T. Soifer;G. Neugebauer;K. Matthews;E. Egami.
The Astronomical Journal (2000)
GOALS: The Great Observatories All-Sky LIRG Survey
L. Armus;J. M. Mazzarella;A. S. Evans;A. S. Evans;J. A. Surace.
Publications of the Astronomical Society of the Pacific (2009)
Explaining the [CII]158um Deficit in Luminous Infrared Galaxies - First Results from a Herschel/PACS Study of the GOALS Sample
T. Diaz-Santos;L. Armus;V. Charmandaris;V. Charmandaris;S. Stierwalt.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
Molecular Gas in the z = 2.565 Submillimeter Galaxy SMM J14011+0252
D T Frayer;R J Ivison;N Z Scoville;A S Evans.
The Astrophysical Journal (1999)
Black hole accretion and star formation as drivers of gas excitation and chemistry in Markarian 231
P. P. van der Werf;K. G. Isaak;K. G. Isaak;R. Meijerink;M. Spaans.
Astronomy and Astrophysics (2010)
The Great Observatories All-Sky LIRG Survey: Comparison of Ultraviolet and Far-Infrared Properties
Justin H. Howell;Lee Armus;Joseph M. Mazzarella;Aaron S. Evans.
arXiv: Astrophysics of Galaxies (2010)
Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies
A. O. Petric;L. Armus;J. Howell;B. Chan.
arXiv: Astrophysics of Galaxies (2010)
Explaining the [C II]157.7 μm Deficit in Luminous Infrared Galaxies—First Results from a Herschel/PACS Study of the GOALS Sample
T. Díaz-Santos;L. Armus;V. Charmandaris;V. Charmandaris;S. Stierwalt.
The Astrophysical Journal (2013)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
California Institute of Technology
California Institute of Technology
University of Crete
Foundation for Research and Technology Hellas
University of Hawaii System
University of Hawaii System
Chalmers University of Technology
National Radio Astronomy Observatory
University of Maryland, College Park
Leiden University
Dublin City University
University of Tehran
University of Maryland, College Park
University of Hull
Pohang University of Science and Technology
University of Chicago
University of Southern California
Genentech
State University of Campinas
Victoria University of Wellington
University of California, Santa Cruz
Virginia Institute of Marine Science
Texas Tech University
Nationwide Children's Hospital
University of Exeter
Norwegian Institute of Public Health