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Gravitational binding energy

Known as: Binding mass, Gravitationally bound 
A gravitational binding energy is the minimum energy that must be added to a system for the system to cease being in a gravitationally bound state. A… 
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Related topics

Related topics

3 relations
Bound stateNumerical integration

Broader (1)

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Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2015
2015
IMPACT OF DUST COOLING ON DIRECT-COLLAPSE BLACK HOLE FORMATION
Observations of quasars at suggest the presence of black holes with a few times . Numerous models have been proposed to explain… 
Highly Cited
2014
Highly Cited
2014
MOST SUB-ARCSECOND COMPANIONS OF KEPLER EXOPLANET CANDIDATE HOST STARS ARE GRAVITATIONALLY BOUND
Using the known detection limits for high-resolution imaging observations and the statistical properties of true binary and line… 
2012
2012
A combined optical and X-ray study of unobscured type 1 active galactic nuclei – II. Relation between X-ray emission and optical spectra
In this second paper in a series of three, we study the properties of the various emission features and underlying continuum in… 
2011
2011
Modeling the flyby anomalies with dark matter scattering: update with additional data and further predictions
We continue our exploration of whether the flyby anomalies can be explained by scattering of spacecraft nucleons from dark matter… 
Highly Cited
2010
Highly Cited
2010
A SPECTROSCOPICALLY CONFIRMED X-RAY CLUSTER AT z = 1.62 WITH A POSSIBLE COMPANION IN THE SUBARU/XMM-NEWTON DEEP FIELD
We report on a confirmed galaxy cluster at z = 1.62. We discovered two concentrations of galaxies at z ∼ 1.6 in the Subaru/XMM… 
Review
2009
Review
2009
ARE NEWLY DISCOVERED H i HIGH-VELOCITY CLOUDS MINIHALOS IN THE LOCAL GROUP?
A set of H i sources extracted from the north Galactic polar region by the ongoing ALFALFA survey has properties that are… 
2004
2004
Keck Spectroscopy of Two Young Globular Clusters in the Merger Remnant NGC 3921
Low-resolution, ultraviolet-to-visual spectra of two candidate globular clusters in the merger remnant NGC 3921 (czLG = 6021 km s… 
2001
2001
Internal kinematics of the TW Hya association of young stars
Thirty one probable kinematic members of the nearby TW Hya association of young stars are selected from the RASSBSC/Tycho-2… 
Review
1999
Review
1999
A WIYN Lithium Survey for Young Stars in the λ Orionis Star-forming Region
We have found 72 pre–main-sequence (PMS) stars near the center of the λ Orionis star-forming region by spectroscopically testing… 
1990
1990
Gasdynamics in interacting and merging galaxies
A three-dimensional model is developed for gas clouds orbiting in the gravitational potential of a galaxy which, at some later… 
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