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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

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
AN AMMONIA SPECTRAL MAP OF THE L1495-B218 FILAMENTS IN THE TAURUS MOLECULAR CLOUD. I. PHYSICAL PROPERTIES OF FILAMENTS AND DENSE CORES
We present deep NH3 observations of the L1495-B218 filaments in the Taurus molecular cloud covering over a 3° angular range using… 
2014
2014
Exceptional AGN-driven turbulence inhibits star formation in the 3C 326N radio-galaxy
We detect bright [CII]158$\mu$m line emission from the radio galaxy 3C 326N at z=0.09, which shows weak star formation ($SFR<0.07… 
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… 
2014
2014
1SWASP J093010.78+533859.5: A POSSIBLE HIERARCHICAL QUINTUPLE SYSTEM
Among quadruples or higher multiplicity stars, only a few doubly eclipsing binary systems have been discovered. They are… 
Highly Cited
2012
Highly Cited
2012
Galactic cold cores - III. General cloud properties
Context. In the project galactic cold cores we are carrying out Herschel photometric observations of cold regions of the… 
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… 
Review
2009
Review
2009
MASSIVE CLUSTERS IN THE INNER REGIONS OF NGC 1365: CLUSTER FORMATION AND GAS DYNAMICS IN GALACTIC BARS
Cluster formation and gas dynamics in the central regions of barred galaxies are not well understood. This paper reviews the… 
Highly Cited
2004
Highly Cited
2004
Resolved Molecular Gas in a Quasar Host Galaxy at Redshift z = 6.42
We present high-resolution Very Large Array (VLA) observations of the molecular gas in the host galaxy of the highest redshift… 
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… 
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