A kinematic and morphological investigation of the asymmetric nebula around the LBV candidate WRA 751
K. Weis *
Received 18 August 1999 / Accepted 3 April 2000
WRA 751 is an evolved massive star in our Galaxy closely resembling Luminous Blue Variable stars (LBVs). It is surrounded by a nitrogen enriched nebula of about 23" diameter. A comparative study of the nebula's morphology and kinematics is presented, it supports-together with spectroscopical evidence-the classification of WRA 751 as a LBV. Images show that the nebula consists of a nearly spherical shell as well as a bipolar-like structure north and south of its main body, the Northern and Southern Caps.
In contrast to the almost spherical appearance of the main body of the nebula, the kinematics shows a deviation even of this part from a classical spherical expansion pattern. From the present data it can be concluded that the main body expands asymmetrically (central expansion velocity km s-1 ), with a thicker shell at the back side. A bump-like structure can be found to the west of the central star. In addition to the main body, bipolar kinematic components can be identified with the morphologically classified Caps. These results put WRA 751 into the class of LBVs which are surrounded by a nebula with bipolar components, albeit considerably less pronounced than, for instance, in the classical bipolar LBVs Car and HR Car.
Key words: stars: individual: WRA 751 stars: evolution stars: mass-loss ISM: bubbles ISM: jets and outflows
* Visiting Astronomer, Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatories, operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation.
Send offprint requests to: K. Weis, Institut für Theoretische Astrophysik, Tiergartenstr. 15, D-69121 Heidelberg, Germany (email@example.com)
Correspondence to: K. Weis, Institut für Theoretische Astrophysik, Tiergartenstr. 15, D-69121 Heidelberg, Germany
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© European Southern Observatory (ESO) 2000
Online publication: June 5, 2000