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The orbital period and system parameters of the recurrent nova T Pyx
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Uthas, Helena, Knigge, Christian and Steeghs, D. (2010) The orbital period and system parameters of the recurrent nova T Pyx. Monthly Notices of the Royal Astronomical Society, Vol.409 (No.1). pp. 237-246. doi:10.1111/j.1365-2966.2010.17046.x ISSN 0035-8711.
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WRAP_STeeghs_T_pyx_1005.5166v1.pdf - Accepted Version Download (743Kb) | Preview |
Official URL: http://dx.doi.org/10.1111/j.1365-2966.2010.17046.x
Abstract
T Pyx is a luminous recurrent nova that accretes at a much higher rate than is expected for its photometrically determined orbital period of about 1.8 h. We here provide the first spectroscopic confirmation of the orbital period, P = 1.8295 h (f = 13.118368 +/- 1.1 x 10(-5) c d(-1)), based on time-resolved optical spectroscopy obtained at the Very Large Telescope and the Magellan telescope. We also derive an upper limit of the velocity semi-amplitude of the white dwarf, K 1 = 17.9 +/- 1.6 kms(-1), and estimate amass ratio of q = 0.20 +/- 0.03. If the mass of the donor star is estimated using the period-density relation and theoretical main-sequence mass-radius relation for a slightly inflated donor star, we find M-2 = 0.14 +/- 0.03 M-circle dot. This implies a mass of the primary white dwarf of M-1 = 0.7 +/- 0.2 M-circle dot. If the white-dwarf mass is > 1 M-circle dot, as classical nova models imply, the donor mass must be even higher. We therefore rule out the possibility that T Pyx has evolved beyond the period minimum for cataclysmic variables. We find that the system inclination is constrained to be i approximate to 10 degrees, confirming the expectation that T Pyx is a low-inclination system. We also discuss some of the evolutionary implications of the emerging physical picture of T Pyx. In particular, we show that epochs of enhanced mass transfer (like the present) may accelerate or even dominate the overall evolution of the system, even if they are relatively short-lived. We also point out that such phases may be relevant to the evolution of cataclysmic variables more generally.
| Item Type: | Journal Article | ||||
|---|---|---|---|---|---|
| Subjects: | Q Science > QB Astronomy | ||||
| Divisions: | Faculty of Science, Engineering and Medicine > Science > Physics | ||||
| Library of Congress Subject Headings (LCSH): | Cataclysmic variable stars | ||||
| Journal or Publication Title: | Monthly Notices of the Royal Astronomical Society | ||||
| Publisher: | Wiley | ||||
| ISSN: | 0035-8711 | ||||
| Official Date: | November 2010 | ||||
| Dates: |
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| Volume: | Vol.409 | ||||
| Number: | No.1 | ||||
| Number of Pages: | 10 | ||||
| Page Range: | pp. 237-246 | ||||
| DOI: | 10.1111/j.1365-2966.2010.17046.x | ||||
| Status: | Peer Reviewed | ||||
| Publication Status: | Published | ||||
| Access rights to Published version: | Restricted or Subscription Access | ||||
| Date of first compliant deposit: | 3 December 2015 | ||||
| Date of first compliant Open Access: | 3 December 2015 | ||||
| Funder: | Science and Technology Facilities Council (Great Britain) (STFC) | ||||
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Data sourced from Thomson Reuters' Web of Knowledge
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