SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 329, 1170 (1998)

Table of Contents

Erratum

HCO + (J = 4-3) mapping of the molecular disk around IRS 7 in Corona Australis

I.M. Anderson 1, J. Harju 1 and L.K. Haikala 1, 2

1 Observatory, P.O. Box 14, FIN-00014 University of Helsinki, Finland
2 Swedish-ESO Submillimetre Telescope, European Southern Observatory, Casilla 19001 Santiago 19, Chile

Astron. Astrophys. 326, 366-372 (1997)

Owing to some unfortunate technical mishap in the final stages of production, Figures 4 and 5 were exchanged and printed upside down.

The correct figures with their captions are reprinted below.

[FIGURE] Fig. 4. The line centre velocity of the HCO [FORMULA] emission line component. The light regions represent blueshifted gas whilst the dark regions represent redshifted gas. The contour levels are from [FORMULA] km s-1 in increments of 0.1 km s-1. The markers have the same significance as in Fig. 2.The beamsize is indicated in the top left of the figure.

[FIGURE] Fig. 5. The line centre velocity of the HCO [FORMULA] emission line component. The light regions represent blueshifted gas whilst the dark regions represent redshifted gas. The contour levels are from [FORMULA] km s-1 in increments of 0.2 km s-1. The markers have the same significance as in Fig. 2. The beamsize is indicated in the top left of the figure. The data are from Paper I.


Table of Contents

© European Southern Observatory (ESO) 1998

Online publication: December 16, 1997
helpdesk.link@springer.de