Separating 21-cm M31 signal from background

Wenlan Miao

doi:10.54254/2753-8818/18/20230450

References

[1]. Results for Messier 31. NASA/IPAC Extragalactic Database

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[3]. Ribas, Ignasi; Jordi, Carme; Vilardell, Francesc; et al. (2005). "First Determination of the Distance and Fundamental Properties of an Eclipsing Binary in the Andromeda Galaxy". Astrophysical Journal Letters. 635 (1): L37–L40.

[4]. "NASA's Hubble Shows Milky Way is Destined for Head-On Collision". NASA. 31 May 2012. Archived from the original on 4 June 2014. Retrieved 12 July 2012.

[5]. Ueda, Junko; Iono, Daisuke; Yun, Min S.; et al. (2014). "Cold molecular gas in merger remnants. I. Formation of molecular gas disks". The Astrophysical Journal Supplement Series. 214 (1): 1

[6]. "M 31, M 32 & M 110". 15 October 2016.

[7]. Arp, Halton (1964). "Spiral Structure in M31". Astrophysical Journal. 139: 1045.

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Cite this article

Miao,W. (2023). Separating 21-cm M31 signal from background. Theoretical and Natural Science,18,302-307.

Data availability

The datasets used and/or analyzed during the current study will be available from the authors upon reasonable request.

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About volume

Volume title: Proceedings of the 2nd International Conference on Computing Innovation and Applied Physics

ISBN：978-1-83558-201-5(Print) / 978-1-83558-202-2(Online)

Editor：Marwan Omar, Roman Bauer

Conference website: https://www.confciap.org/

Conference date: 25 March 2023

Series: Theoretical and Natural Science

Volume number: Vol.18

ISSN：2753-8818(Print) / 2753-8826(Online)

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