Sentence examples for metal masses from inspiring English sources

The band's carefully constructed anti-image – anonymous, faceless, shadowy figures fronted by a masked, mitre-sporting demon – also ensures they stand apart from the identikit metal masses.

As for the remnant and metal masses, the data are taken from van den Hoek and Groenewegen (1997) for AGB stars with a mass range 1 7 M⊙ and metallicities Z = (5.0 × 10−2, 0.2, 0.4, 1.0) Z⊙, and from Woosley and Weaver (1995) for SNe II with a mass range 12 40 M⊙ and metallicities Z = (5.0 × 10−2,0.1, 1.0) Z⊙.

Finland in particular, with metal being more mainstream there than anywhere in the world, has held popular Metal Masses picked up by the Lutheran former state church since 2006.

Fig. 7. Time evolution of metallicity (metal mass fraction in the ISM; dashed line) and dust-to-gas mass ratio (other lines) for the fiducial case (Table 1).

Furthermore, to describe the dust evolution precisely, our model takes into account the age and metallicity (the ratio of metal mass to ISM mass) dependence of the sources of dust.

We adopt the metal mass fraction (so-called metallicity) in the Sun of Z⊙ = 0.02 (Anders and Grevesse, 1989) conventionally, although recent measurements suggest a smaller value of 0.0134 (Asplund et al., 2009).

Using the IMF, ϕ(m), and the star-formation rate, S t), we can express the metal yield as (10 where m Z is the metal mass ejected from a star with mass m and metallicity Z, and t′ is given by Eq. (9).

It's impossible to guess what the interior is like by exploring the outside of this huge, reddish metal mass that fills most of the biggest space in the warehouse-like Gagosian Britannia Street gallery near King's Cross.

In this work, the generator structure of composite cantilever with nickel metal mass is devised.

Fig. 2. Ejected metal mass fraction, m Z /m, as a function of the initial stellar mass, m.

Time evolution of the ratio of dust mass produced by stars to metal mass ejected by stars.