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The Geometry of and Mass Accretion Rate through the Maser Accretion Disk in NGC 4258

ASTROPHYSICAL JOURNAL, no. 2 (2005): 719-738

Cited: 83|Views26

Abstract

A maximum likelihood analysis of the NGC 4258 maser positions and velocities reveals a similar to 2 sigma deviation from Keplerian motion in the projected rotation curve of the high-velocity features, corresponding to a similar to 9 km s(-1), or 0.8%, flattening of the LOS velocities with respect to Keplerian motion over the range of the ...More

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