dc.creator |
Turner, David Gerald, 1945- |
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dc.creator |
Kovtyukh, V. V. |
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dc.creator |
Usenko, I. A. |
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dc.creator |
Gorlova, N. I. |
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dc.date.accessioned |
2018-02-23T16:08:42Z |
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dc.date.available |
2018-02-23T16:08:42Z |
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dc.date.issued |
2013-01-01 |
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dc.identifier.issn |
2041-8205 |
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dc.identifier.uri |
http://library2.smu.ca/handle/01/27287 |
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dc.description |
Publisher's version/PDF |
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dc.description.abstract |
<p>A previously derived photometric parallax of 10.10 ± 0.20 mas, d = 99 ± 2 pc, is confirmed for Polaris by a spectroscopic parallax derived using line ratios in high dispersion spectra for the Cepheid. The resulting estimates for the mean luminosity of ⟨M<sub>V</sub>⟩ = −3.07 ± 0.01 s.e., average effective temperature of ⟨T<sub>eff</sub>⟩ = 6025 ± 1 K s.e., and intrinsic color of (⟨B⟩ − ⟨V⟩)<sub>0</sub> = +0.56 ± 0.01 s.e., which match values obtained previously from the photometric parallax for a space reddening of E<sub>B−V</sub> = 0.02 ± 0.01, are consistent with fundamental mode pulsation for Polaris and a first crossing of the instability strip, as also argued by its rapid rate of period increase. The systematically smaller <em>Hipparcos</em> parallax for Polaris appears discrepant by comparison.</p> |
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dc.description.provenance |
Submitted by Betty McEachern (betty.mceachern@smu.ca) on 2018-02-23T16:08:42Z
No. of bitstreams: 1
Turner_David_G_article_2013_b.pdf: 222490 bytes, checksum: b979249f2feb097d12ac841bd42bbe98 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2018-02-23T16:08:42Z (GMT). No. of bitstreams: 1
Turner_David_G_article_2013_b.pdf: 222490 bytes, checksum: b979249f2feb097d12ac841bd42bbe98 (MD5)
Previous issue date: 2013 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
IOP Publishing Limited |
en_CA |
dc.relation.uri |
https://dx.doi.org/10.1088/2041-8205/762/1/L8 |
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dc.subject.lcsh |
Polestar |
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dc.subject.lcsh |
Cepheids |
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dc.title |
The pulsation mode of the Cepheid Polaris |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Astrophysical Journal Letters 762(1), L8. (2013) |
en_CA |