The warp in the sub-parsec-scale molecular disk in NGC 4258 as an explanation for persistent asymmetries in the water maser spectrum.

Details The warp in the sub-parsec-scale molecular disk in NGC 4258 as an explanation for persistent asymmetries in the water maser spectrum. The warp in the sub-parsec-scale molecular disk in NGC 4258 as an explanation for persistent asymmetries in the water maser spectrum.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996baas...28..846h&link_type=gif

Bulletin of the Astronomical Society, Vol. 28, No. 2, p. 846

Astronomy and Astrophysics

Astronomy

Active Galaxies: Water Masers, Active Galaxies: Galactic Disks

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