Mini-Spiral at the Galactic Center: A Link between its Structure and the Value of a Central Point Mass
The innermost 2 pc contain a rotating ring (“circumnuclear disk”) of molecular gas, neutral hydrogen, and dust with an embedded H II region called Sgr A West; a dense stellar cluster; and a compact nonthermal radio source Sgr A ∗ (for a recent review, see Blitz et al. 1993). The clumped, spiral-shap...
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Veröffentlicht in: | Symposium - International Astronomical Union 1996, Vol.169, p.241-246 |
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Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The innermost 2 pc contain a rotating ring (“circumnuclear disk”) of molecular gas, neutral hydrogen, and dust with an embedded H II region called Sgr A West; a dense stellar cluster; and a compact nonthermal radio source Sgr A
∗
(for a recent review, see Blitz
et al.
1993). The clumped, spiral-shaped morphology of Sgr A West, sometimes called lthe mini-spiral”, has been a subject of numerous speculations concerning its origin (for a review, see Genzel & Townes 1987). Lacy
et al.
(1991) demonstrated that both the kinematics and shape of a part of Sgr A West can be fairly well approximated using an one-armed density-wave model. |
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ISSN: | 0074-1809 |
DOI: | 10.1017/S0074180900229744 |