Answer to Question #203525 in Astronomy | Astrophysics for Laxminarayan

Question

This problem requires you to read the following recently published

scientific article:

Measuring the ionisation fraction in a jet from a massive protostar.

Fedriani, R., Caratti o Garatti, A., Purser, S.J.D. et al. Nat Commun

10, 3630 (2019).

Link: https://www.nature.com/articles/s41467-019-11595-x.pdf

Answer the following questions related to this article:

(a) Why are massive stars important for the development of the

universe?

(b) How can the ionised part of jets be observed?

(c) What kind of region is G35.2N? Describe how it is structured.

(d) What is the ionisation fraction χe and how do the authors

calculate its value?

(e) How is the mass-loss rate being determined for knots K3 and K4?

Why not for K1 and K2?

(f) Why is the ionisation fraction so small for G35.2N?

Answer 1

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