Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-25T17:24:54.828Z Has data issue: false hasContentIssue false

A 500 kpc HI Tail of the Virgo Pair NGC4532/DDO137 Detected by ALFALFA

Published online by Cambridge University Press:  01 June 2007

Rebecca A. Koopmann*
Affiliation:
Department of Physics and Astronomy, Union College, Schenectady, NY 12308, email: [email protected] National Astronomy and Ionosphere Center†, Space Sciences Building, Cornell University, Ithaca NY 14853
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

HI observations of the Virgo Cluster pair NGC 4532/DDO 137, conducted as part of the Arecibo Legacy Fast ALFA Survey, reveal an HI feature extending ~500kpc to the southwest. The structure has a total mass of up to 7 x 108M, equivalent to 10% of the pair HI mass. Optical R imaging reveals no counterparts to a level of 26.5 mag arcsec−2. The structure is likely the result of galaxy harassment.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Bekki, K., Koribalski, B. S., & Kilborn, V. A. 2005, MNRAS 363, L21CrossRefGoogle Scholar
Boselli, A. & Gavazzi, G. 2006, PASP, 118, 517CrossRefGoogle Scholar
Giovanelli, et al. 2005a, AJ, 130, 2598CrossRefGoogle Scholar
Haynes, Giovanelli, & Kent, 2007 ApJ, 665, 19CrossRefGoogle Scholar
Hoffman, G. L. et al. 1993, AJ, 106, 39CrossRefGoogle Scholar
Hoffman, G. L. et al. 1999, AJ, 117, 811CrossRefGoogle Scholar
Kent, et al. 2007 ApJ, 665, 15CrossRefGoogle Scholar