The Planetary Nebula M2-9: Balmer Line Profiles of the Nuclear Region

Astronomy and Astrophysics – Astronomy

Scientific paper

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Planetary Nebulae, Radiative Transfer, Planetary Nebulae, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

The central source of M2-9 shows an exceptionally intense and wide
Hα line, and anomalous Balmer profiles. We attempt to fit the
complex line profiles of the Balmer series by solving the line transfer
in a very dense medium surrounding the central star.

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