{ "id": "1004.4799", "version": "v1", "published": "2010-04-27T13:34:09.000Z", "updated": "2010-04-27T13:34:09.000Z", "title": "High Resolution Spectroscopy of the Planetary Nebulae PM1-242, PM1-318 and PM1-322", "authors": [ "L. F. Miranda", "R. Vázquez", "M. A. Guerrero", "C. B. Pereira", "E. Iñiguez-Garín" ], "comment": "4 pages, 3 figures, accepted for publication in PASA", "categories": [ "astro-ph.SR" ], "abstract": "We have recently confirmed the planetary nebula (PN)nature of PM1-242, PM1-318 and PM1-322. Here we present high-resolution long-slit spectra of these three PNe in order to analyze their internal kinematics and to investigate their physical structure. PM1-242 is a tilted ring and not an elliptical PN as suggested by direct images. The object is probably related to ring-like PNe and shows an unusual point-symmetric brightness distribution in the ring. PM1-318 is a pole-on elliptical PN, instead of a circular one as suggested by direct images. PM1-322 is spatially unresolved and its spectrum shows large differences between the forbidden lines and H$\\alpha$ profiles, with the latter showing a double-peaked profile and relatively extended wings (FWZI $\\sim$ 325 km\\,s$^{-1}$). These properties are found in other PNe that are suspected to host a symbiotic central star.", "revisions": [ { "version": "v1", "updated": "2010-04-27T13:34:09.000Z" } ], "analyses": { "keywords": [ "high resolution spectroscopy", "planetary nebula", "unusual point-symmetric brightness distribution", "direct images", "high-resolution long-slit spectra" ], "tags": [ "journal article" ], "publication": { "doi": "10.1071/AS09029", "journal": "Publications of the Astronomical Society of Australia", "year": 2010, "month": "May", "volume": 27, "number": 2, "pages": 199 }, "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 853113, "adsabs": "2010PASA...27..199M" } } }