Neutral Hydrogen Asymmetry in the Galaxy M101 as Evidence for Tidal Effects-Reference-Cited by-同舟云学术

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Neutral Hydrogen Asymmetry in the Galaxy M101 as Evidence for Tidal Effects

Published:1969-02 Issue:5180 Volume:221 Page:531-533
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

BEALE J. S.,DAVIES R. D.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/221531a0.pdf

Reference13 articles.

1. Gottesman, S. T., thesis, Univ. Manchester (1967).

2. de Jager, G., thesis, Univ. Manchester (1967).

3. de Vaucouleurs, G., and A., Reference Catalogue of Bright Galaxies (Univ. Texas Press, 1964).

4. Roberts, M. S., Astrophys. J., 144, 639 (1966).

5. Arp, H., IAU Symp. No. 20, The Galaxy and the Magellanic Clouds (edit. by Kerr, F. J., and Rodgers, A. W.), 219 (1964).

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1. A Dynamic Galaxy: Stellar Age Patterns across the Disk of M101;The Astrophysical Journal;2024-01-29

2. Shape Asymmetries and the Relation between Lopsidedness and Radial Alignment in Simulated Galaxies;The Astrophysical Journal;2024-01-01

3. Lopsidedness as a tracer of early galactic assembly history;Monthly Notices of the Royal Astronomical Society;2023-09-04

4. Deep Narrowband Photometry of the M101 Group: Strong-line Abundances of 720 H ii Regions;The Astrophysical Journal;2022-12-01

5. Discovery of Extraplanar H i Clouds and a H i Tail in the M101 Galaxy Group with FAST;The Astrophysical Journal;2021-11-01

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