Spectral analysis of PG 1034+001, the exciting star of Hewett 1

AbstractPG 1034+001 is an extremely hot, helium-rich DO-type star that excites the planetary nebula Hewett 1 and large parts of the surrounding interstellar medium. We present preliminary results of an ongoing spectral analysis by means of non-LTE model atmospheres that consider most elements from hydrogen to nickel. This analysis is based on high-resolution ultraviolet (FUSE, IUE) and optical (VLT/UVES, Keck) data. The results are compared with those of PG 1034+001's spectroscopic twin, the DO star PG 0038+199.

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Spectral analysis of the sdO K 648, the exciting star of the planetary nebula Ps 1 in the globular cluster M 15 (NGC 7078)

Astronomy and Astrophysics ◽

10.1051/0004-6361:20011535 ◽

2002 ◽

Vol 381 (3) ◽

pp. 1007-1014 ◽

Cited By ~ 32

Author(s):

T. Rauch ◽

U. Heber ◽

K. Werner

Keyword(s):

Spectral Analysis ◽

Globular Cluster ◽

Planetary Nebula ◽

Exciting Star

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Signature of Transpressional Tectonics in the Holocene Stratigraphy of Lake Azuei, Haiti: Preliminary Results From a High-Resolution Subbottom Profiling Survey

10.1002/essoar.10500011.1 ◽

2018 ◽

Author(s):

Marie-Helene Cormier ◽

Heather Sloan ◽

Dominique Boisson ◽

Britta Brown ◽

Kelly Guerrier ◽

...

Keyword(s):

High Resolution ◽

The Holocene ◽

Preliminary Results ◽

Holocene Stratigraphy ◽

Subbottom Profiling

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Spatial lattice filter for high-resolution spectral analysis of array data

IEE Proceedings F Communications Radar and Signal Processing ◽

10.1049/ip-f-1.1983.0047 ◽

1983 ◽

Vol 130 (3) ◽

pp. 279 ◽

Cited By ~ 9

Author(s):

K.C. Sharman ◽

T.S. Durrani

Keyword(s):

Spectral Analysis ◽

High Resolution ◽

Array Data ◽

Lattice Filter ◽

Spatial Lattice

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High‐Resolution X‐Ray Image of the Hydrogen‐deficient Planetary Nebula Abell 30

The Astrophysical Journal ◽

10.1086/304196 ◽

1997 ◽

Vol 482 (2) ◽

pp. 891-896 ◽

Cited By ~ 23

Author(s):

You‐Hua Chu ◽

Thomas H. Chang ◽

Gail M. Conway

Keyword(s):

High Resolution ◽

Planetary Nebula ◽

X Ray

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Spectral Analysis of the High Resolution ECG: Current Concepts and Future Directions

Pacing and Clinical Electrophysiology ◽

10.1111/j.1540-8159.1994.tb01411.x ◽

1994 ◽

Vol 17 (3) ◽

pp. 446-450 ◽

Cited By ~ 3

Author(s):

RALPH HABERL ◽

PETER STEINBIGLER ◽

GERHARD JILGE

Keyword(s):

Spectral Analysis ◽

High Resolution ◽

Future Directions

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High-resolution spectral analysis methods for self-potential data inversion

10.1190/segam2015-5810869.1 ◽

2015 ◽

Cited By ~ 4

Author(s):

Payal Rani* ◽

Rosa Di Maio ◽

Ester Piegari

Keyword(s):

Spectral Analysis ◽

High Resolution ◽

Data Inversion ◽

Analysis Methods ◽

Self Potential

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Morphokinematic properties of the 21 micron source IRAS 22272+5435

Proceedings of the International Astronomical Union ◽

10.1017/s174392131201191x ◽

2011 ◽

Vol 7 (S283) ◽

pp. 458-459

Author(s):

Jun-ichi Nakashima ◽

Sun Kwok ◽

Bosco H. K. Yung ◽

Yong Zhang ◽

Nico Koning ◽

...

Keyword(s):

High Resolution ◽

Angular Size ◽

Mid Infrared ◽

Preliminary Results ◽

Molecular Envelope

AbstractWe obtained a high-resolution CO map of IRAS 22272+5435 in the CO J = 2–1 line using CARMA. The target exhibits a second biggest angular size of the circumstellar molecular envelope among known 21 μm sources. In the preliminary results, we found that the CO properties of IRAS 22272+5435 is clearly different from those of IRAS 07134+1005, which is another well-investigated 21 μm source. For example, elongations seen in the mid-infrared and CO images are extended in mutually perpendicular directions, although in case of IRAS 07134+1005 the CO feature coincides well with the mid-infrared structure.

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