What is he best known for?
The fields of study he is best known for:
- Astronomy
- Astrophysics
- Galaxy
His scientific interests lie mostly in Astrophysics, Astronomy, Molecular cloud, Stars and Star formation.
With his scientific publications, his incorporates both Astrophysics and Outflow.
His Astronomy study focuses mostly on Orion Nebula, Young stellar object, Herbig–Haro object, Nebula and Protostar.
His Molecular cloud research includes elements of Jet, Luminosity, Interstellar medium, Turbulence and Emission spectrum.
His work on Accretion and T Tauri star as part of general Stars study is frequently linked to Excitation and Isothermal process, bridging the gap between disciplines.
His studies in Star formation integrate themes in fields like X-ray binary and Stellar evolution.
His most cited work include:
- The bell laboratories H I survey (828 citations)
- Clouds, filaments, and protostars: The Herschel Hi-GAL Milky Way (649 citations)
- Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way (648 citations)
What are the main themes of his work throughout his whole career to date?
His primary areas of study are Astrophysics, Astronomy, Stars, Star formation and Molecular cloud.
His multidisciplinary approach integrates Astrophysics and Outflow in his work.
In his research on the topic of Astronomy, Bow shock is strongly related with Jet.
His work carried out in the field of Stars brings together such families of science as Luminosity, Supernova and Infrared.
He has included themes like Spectral line, Star cluster, Star and Stellar evolution in his Star formation study.
His Molecular cloud research integrates issues from Line, Radiative transfer, Interstellar medium and Emission spectrum.
He most often published in these fields:
- Astrophysics (88.37%)
- Astronomy (62.30%)
- Stars (37.82%)
What were the highlights of his more recent work (between 2014-2021)?
- Astrophysics (88.37%)
- Astronomy (62.30%)
- Stars (37.82%)
In recent papers he was focusing on the following fields of study:
Astrophysics, Astronomy, Stars, Star formation and Galaxy are his primary areas of study.
In the subject of general Astrophysics, his work in Molecular cloud, Supernova and Milky Way is often linked to Outflow, thereby combining diverse domains of study.
His study in the fields of Star cluster, Orion Nebula and Extinction under the domain of Stars overlaps with other disciplines such as Excitation.
His research investigates the link between Star formation and topics such as Turbulence that cross with problems in Solenoidal vector field.
His Protostar study which covers Spectral line that intersects with Telescope.
His study looks at the relationship between Nebula and fields such as Jet, as well as how they intersect with chemical problems.
Between 2014 and 2021, his most popular works were:
- Illuminating gravitational waves: A concordant picture of photons from a neutron star merger (432 citations)
- Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues. First data release for Inner Milky Way: +68{\deg}> l > -70{\deg} (180 citations)
- Hi-GAL, the Herschel infrared Galactic Plane Survey: Photometric maps and compact source catalogues: First data release for the inner Milky Way: +68° ≥ l ≥ -70° (180 citations)
In his most recent research, the most cited papers focused on:
- Astronomy
- Astrophysics
- Galaxy
His scientific interests lie mostly in Astrophysics, Stars, Star formation, Astronomy and Galaxy.
In his works, John Bally undertakes multidisciplinary study on Astrophysics and Outflow.
His work on Protoplanetary disk and Orion Nebula as part of general Stars research is often related to Excitation, thus linking different fields of science.
The various areas that John Bally examines in his Star formation study include Galactic Center, Star cluster, Stellar evolution, Turbulence and Line-of-sight.
Astronomy is often connected to Jet in his work.
Luminous red nova is closely connected to Infrared in his research, which is encompassed under the umbrella topic of Galaxy.
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.
