Bondi accretion
accretion of matter within the interstellar medium
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Bondi accretion
Summary
Bondi accretion is a physical law[1]. It draws 49 Wikipedia views per month (physical_law category, ranking #83 of 113).[2]
Key Facts
- Bondi accretion's instance of is recorded as physical law[3].
- Hermann Bondi is named after Bondi accretion[4].
- Bondi accretion's subclass of is recorded as accretion[5].
- Bondi accretion's Freebase ID is recorded as /m/05b4b65[6].
- Bondi accretion's different from is recorded as Bondi–Hoyle–Lyttleton accretion[7].
- Bondi accretion's defining formula is recorded as \dot{M} \simeq \pi R^2 \rho v[8].
- Bondi accretion's studied by is recorded as astrophysics[9].
- Bondi accretion's Unified Astronomy Thesaurus ID is recorded as 174[10].
- Bondi accretion's maintained by WikiProject is recorded as WikiProject Mathematics[11].
- Bondi accretion's Microsoft Academic ID is recorded as 2779755411[12].
Why It Matters
Bondi accretion draws 49 Wikipedia views per month (physical_law category, ranking #83 of 113).[2] It has Wikipedia articles in 9 language editions, a strong signal of global cultural recognition.[13] It is known by 4 alternative names across languages and contexts.[14]