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The use of body mass loss to estimate metabolic rate in birds
Comparative Biochemistry and Physiology Part A: Molecular & Integrative Physiology, 2011During starvation, energy production occurs at the expense of body reserve utilisation which results in body mass loss. Knowing the role of the fuels involved in this body mass loss, along with their energy density, can allow an energy equivalent of mass loss to be calculated. Therefore, it is possible to determine daily energy expenditure (DEE) if two
Steven J, Portugal, Magella, Guillemette
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The Mass Loss Rate of a Candle during Burning
Advanced Materials Research, 2014The presented article deals with setting the effect of paraffin candles and thickness of their wick on the speed of candle weight loss. The paraffin candles with gauge of 1.8 to 6.8 cm and wick thickness of 1.5 to 3 mm were subjected to the test. The test procedure was based on setting the tested candles on a digital scales with resolution of 0,001 g ...
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Mass loss rate of the zodiacal dust cloud
The Moon and the Planets, 1983The mass loss rate of the zodiacal dust cloud near the Sun has been estimated on the basis of the orbital behaviour of circumsolar dust grains suffering sublimation. It is found that the solar dust ring located at 4 solar radii from the Sun, which consists of grains whose inward spiraling due to the Poynting-Robertson effect is stopped by the influence
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On the disk wind mass loss rates in QSOs
New Astronomy, 2015Abstract We derive here a relatively simple expression for the total wind mass loss rates in QSOs within the accretion disk wind scenario. We show that the simple expression derived here for QSO disk wind mass loss rate is in a very good agreement with the more “exact” values obtained through significantly more complex and detailed numerically ...
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Rate of Mass-Loss in the Hertzsprung-Russell Diagram
1987We have collected literature data on rates of mass-loss \({\dot M}\) for 264 0 through M-type stars and a number of stars of other types. It appears possible to develop log(- \(\left( { - \dot M} \right)\) ) into a series of Chebychev polynomia of the first kind in log Teff and log (L/L⨀) and their cross products.
Cornelis de Jager +2 more
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The Disc Structure and Mass Loss Rates of Be Stars
1986IRAS observations of four well-known Be stars, α Eri, φ Per, δ Cen and χ Oph are used to derive the density structure of the circumstellar discs and the mass loss rates. α Eri shows no sign of IR excess up to λ = 60 µm, but the other three have excesses in the order of a factor 10 to 70, caused by free-free radiation from the disc.
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Integrated mass-loss of evolved stars in M4 using asteroseismology
Monthly Notices of the Royal Astronomical Society, 2022Madeline Howell +2 more
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Weight Loss Strategies and the Risk of Skeletal Muscle Mass Loss
Nutrients, 2021David Mccarthy, A Berg
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Frontal ablation and mass loss of the Patagonian icefields
Earth and Planetary Science Letters, 2021Masahiro Minowa +2 more
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Mass loss and the Eddington parameter: a new mass-loss recipe for hot and massive stars
Monthly Notices of the Royal Astronomical Society, 2020J M Bestenlehner
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