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Astrometry with Hubble Space Telescope Fine Guidance Sensor 3: The Parallax of the Cataclysmic Variable RW Triangulum
Astrophysics · Submitted 21 May 1999
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim This determination puts the distance of RW Tri at 341, one of the most distant objects with a direct parallax measurement.
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The abstract, sentence by sentence
RW Triangulum (RW Tri) is a 13th magnitude Nova-like Cataclysmic Variable star with an orbital period of 0.2319 days (5.56 hours). Infrared observations of RW Tri indicate that its secondary is most likely a late K-dwarf. Past analyses predicted a distance of 270 parsec, derived from a black-body fit to spectrum of the central part of the disk. Recently completed Hubble Space Telescope Fine Guidance Sensor interferometric observations allow us to determine the first trigonometric parallax to RW Tri. This determination puts the distance of RW Tri at 341, one of the most distant objects with a direct parallax measurement.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | RW Triangulum (RW Tri) is a 13th magnitude Nova-like Cataclysmic Variable star with an orbital period of 0.2319 days (5.56 hours). | background 1.00 | 0.16 | 0.02 | asserted 1.00 |
| s1 | Infrared observations of RW Tri indicate that its secondary is most likely a late K-dwarf. | background 0.98 | 0.19 | 0.02 | hedged possibility 1.00 |
| s2 | Past analyses predicted a distance of 270 parsec, derived from a black-body fit to spectrum of the central part of the disk. | background 0.99 | 0.05 | 0.02 | asserted 0.98 |
| s3 | Recently completed Hubble Space Telescope Fine Guidance Sensor interferometric observations allow us to determine the first trigonometric parallax to RW Tri. | contribution 0.50 | 0.88 | 0.14 | asserted 0.91 |
| s4 | This determination puts the distance of RW Tri at 341, one of the most distant objects with a direct parallax measurement. | result 0.98 | 0.94 | 0.89 | asserted 1.00 |
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The paper
Original abstract
RW Triangulum (RW Tri) is a 13th magnitude Nova-like Cataclysmic Variable star with an orbital period of 0.2319 days (5.56 hours). Infrared observations of RW Tri indicate that its secondary is most likely a late K-dwarf. Past analyses predicted a distance of 270 parsec, derived from a black-body fit to spectrum of the central part of the disk. Recently completed Hubble Space Telescope Fine Guidance Sensor interferometric observations allow us to determine the first trigonometric parallax to RW Tri. This determination puts the distance of RW Tri at 341, one of the most distant objects with a direct parallax measurement.
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