Zobrazeno 1 - 10
of 65
pro vyhledávání: '"Hugo E. Schwarz"'
Autor:
Hugo E. Schwarz, Hektor Monteiro
Publikováno v:
Exacta. 4:281-288
Publikováno v:
The Astrophysical Journal. 675:380-388
We show that the inclination to the line of sight of bipolar planetary nebulae strongly affects some of their observed properties. We model these objects as having a dusty equatorial density enhancement that produces extinction that varies with the v
Autor:
Hugo E. Schwarz, Hektor Monteiro
Publikováno v:
The Astrophysical Journal. 648:430-434
Continuing our series of papers on the three-dimensional (3-D) structures of and accurate distances to Planetary Nebulae (PNe), we present our study of the planetary nebula NGC6781. For this object we construct a 3-D photoionization model and, using
Autor:
Hektor Monteiro, Hugo E. Schwarz
Publikováno v:
Exacta, Vol 4, Iss 2, Pp 281-288 (2006)
Continuing our series of papers on the three-dimensional (3-D) structures of and accurate distances to Planetary Nebulae (PNe), we present our study of the planetary nebula NGC6781. For this object we construct a 3-D photoionization model and, using
Publikováno v:
The Astrophysical Journal. 620:321-329
We present the results of a spatio-kinematic study of the planetary nebula Menzel 1 using spectro-photometric mapping and a 3-D photoionization code. We create several 2-D emission line images from our long-slit spectra, and use these to derive the l
Publikováno v:
The Astrophysical Journal. 609:194-202
Autor:
Kjell Eriksson, Hans Olofsson, Tim Gledhill, Hugo E. Schwarz, Bengt Gustafsson, D. González Delgado
Publikováno v:
University of Hertfordshire
Imaging polarimetry has been used to study the extended, detached circumstellar shells around the bright carbon stars R Scl and U Ant. The observations were done in two narrow band filters centred on the resonance lines of neutral K and Na, but much
Publikováno v:
The Astrophysical Journal. 553:211-218
New Hubble Space Telescope images and Cerro Tololo Inter-American Observatory echelle spectra of the nebula around the symbiotic Mira Henize 2-104 are presented. The nebula consists of two nested hourglass-shaped structures and a collimated polar jet
Publikováno v:
The Astronomical Journal. 119:1339-1344
The planetary nebula M2-9 has drastically changed its shape since its discovery by Minkwoski. Although the outline of the nebula seems to be stationary, most of the knots and bright features (N1, N2, S1, and S2) have moved laterally from the west to
Publikováno v:
Symposium - International Astronomical Union. 177:409-412
Circumstellar emission in the Na I and K I resonance lines has been detected from three carbon stars using high-resolution spectroscopy. Some properties of the circumstellar envelopes are discussed.