Turbulent power spectrum in warm and cold neutral medium using the Galactic H i21 cm emission
Author:
Affiliation:
1. National Centre For Radio Astrophysics, Post Bag 3, Ganeshkhind, Pune 411 007, India
2. Department of Physics, Indian Institute of Science, Bangalore 560012, India
Funder
Infosys Foundation
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/483/3/3437/27242807/sty3342.pdf
Reference36 articles.
1. A high sensitivity Hi survey of the sky at δ ≤ -25°
2. A high sensitivity HI survey of the sky at $\mathsf{\delta \le -25 \degr}$
3. DHIGLS: DRAO H i INTERMEDIATE GALACTIC LATITUDE SURVEY
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