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Effect of body fat mass loss on prognosis of radical resection for pancreatic ductal adenocarcinoma based on bioelectrical impedance analysis. [PDF]
BMC SurgShibata Y +12 more
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rGdf5, an unexpected treatment against age-related muscle mass loss
, 2019 Sestina Falcone +7 more
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Hydrogen Deficiency and Mass Loss
Symposium - International Astronomical Union, 1979Some conclusions concerning the luminous hydrogen-deficient stars are presented, as is also a list of 45 such objects.
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Symposium - International Astronomical Union, 1970
In this summary we shall attempt to evaluate the mass loss from several kinds of high luminosity stars, especially planetary nebulae, OB supergiants and M giants and supergiants. The purpose is to give an observational basis for the discussion of the mechanism of mass loss and of the consequences of stellar mass loss for the interstellar medium and for
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In this summary we shall attempt to evaluate the mass loss from several kinds of high luminosity stars, especially planetary nebulae, OB supergiants and M giants and supergiants. The purpose is to give an observational basis for the discussion of the mechanism of mass loss and of the consequences of stellar mass loss for the interstellar medium and for
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Nature Climate Change, 2020
Gravity-based estimates of mass change have been extended by the recently launched GRACE Follow-On Satellites. The satellite record, combined with regional climate models, reveals that the Greenland Ice Sheet had lower mass loss in 2017–2018, only to return to a record-breaking mass loss in the summer of 2019.
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Gravity-based estimates of mass change have been extended by the recently launched GRACE Follow-On Satellites. The satellite record, combined with regional climate models, reveals that the Greenland Ice Sheet had lower mass loss in 2017–2018, only to return to a record-breaking mass loss in the summer of 2019.
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2001
The problem of mass loss is described in the context of non-linear radial pulsations of luminous stars. The numerical requirements of such computations are briefly discussed. The first example is devoted to models of dust-driven winds from AGB-stars. The second part illustrates numerical computations of LBVs in some detail to understand the long term ...
Ernst A. Dorfi +2 more
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The problem of mass loss is described in the context of non-linear radial pulsations of luminous stars. The numerical requirements of such computations are briefly discussed. The first example is devoted to models of dust-driven winds from AGB-stars. The second part illustrates numerical computations of LBVs in some detail to understand the long term ...
Ernst A. Dorfi +2 more
openaire +1 more source