Results 281 to 290 of about 1,250,119 (305)
Some of the next articles are maybe not open access.
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 ...
openaire +1 more source
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
openaire +1 more source
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 ...
openaire +1 more source
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
openaire +1 more source
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.
openaire +1 more source
Integrated mass-loss of evolved stars in M4 using asteroseismology
Monthly Notices of the Royal Astronomical Society, 2022Madeline Howell +2 more
exaly
Weight Loss Strategies and the Risk of Skeletal Muscle Mass Loss
Nutrients, 2021David Mccarthy +2 more
exaly
Frontal ablation and mass loss of the Patagonian icefields
Earth and Planetary Science Letters, 2021Masahiro Minowa +2 more
exaly
On the nature of massive helium star winds and Wolf–Rayet-type mass-loss
Monthly Notices of the Royal Astronomical Society, 2020A A C Sander +2 more
exaly