排序方式: 共有86条查询结果,搜索用时 15 毫秒
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New species of Mentzelia and Phacelia are described from northwestern New Mexico, USA, as Mentzelia todiltoensis , N. Duane Atwood & Stanley L. Welsh, and Phacelia sivinskii N. D. Atwood, sp. nov. The new Mentzelia is compared to M. humilis based on similarities in seed, fruit, leaf, and flower morphology and to M. memorabalis in stem, leaf, and fruit morphology. Phacelia sivinskii is compared to P. constancei N. D. Atwood on the basis of seed, leaf, and flower morphology. 相似文献
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Stanley L. Welsh 《西北部美国博物学家》2011,58(1)
This is a summary monograph of the hanging gardens as they occur in the Colorado River and Virgin River portion of the Colorado Plateau in Utah. Discussed in this paper are the hanging gardens, their geography, geomorphology, aspects of distribution and diversity, and principal vascular and algal plant species. Animal trapping studies and pland productivity aspects are reviewed. 相似文献
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The paper presents an annotated list of 851 taxa in 358 genera and 80 families. Threatened and endangered plants are enumerated. 相似文献
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Astragalus atwoodii Welsh and Thorne is named and described on the basis of materials collected on the Kaibab Plateau in Coconino County, Arizona. 相似文献
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Discussed are relationships of the species within Astragalus section Conjuncti; A. conjunctus var. rickardii Welsh, Beck, & Caplow var. nov. is proposed. 相似文献
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Stanley L. Welsh 《西北部美国博物学家》2011,43(2)
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Welsh WF Orosz JA Carter JA Fabrycky DC Ford EB Lissauer JJ Prša A Quinn SN Ragozzine D Short DR Torres G Winn JN Doyle LR Barclay T Batalha N Bloemen S Brugamyer E Buchhave LA Caldwell C Caldwell DA Christiansen JL Ciardi DR Cochran WD Endl M Fortney JJ Gautier TN Gilliland RL Haas MR Hall JR Holman MJ Howard AW Howell SB Isaacson H Jenkins JM Klaus TC Latham DW Li J Marcy GW Mazeh T Quintana EV Robertson P Shporer A Steffen JH Windmiller G Koch DG Borucki WJ 《Nature》2012,481(7382):475-479
Most Sun-like stars in the Galaxy reside in gravitationally bound pairs of stars (binaries). Although long anticipated, the existence of a 'circumbinary planet' orbiting such a pair of normal stars was not definitively established until the discovery of the planet transiting (that is, passing in front of) Kepler-16. Questions remained, however, about the prevalence of circumbinary planets and their range of orbital and physical properties. Here we report two additional transiting circumbinary planets: Kepler-34 (AB)b and Kepler-35 (AB)b, referred to here as Kepler-34 b and Kepler-35 b, respectively. Each is a low-density gas-giant planet on an orbit closely aligned with that of its parent stars. Kepler-34 b orbits two Sun-like stars every 289?days, whereas Kepler-35 b orbits a pair of smaller stars (89% and 81% of the Sun's mass) every 131?days. The planets experience large multi-periodic variations in incident stellar radiation arising from the orbital motion of the stars. The observed rate of circumbinary planets in our sample implies that more than ~1% of close binary stars have giant planets in nearly coplanar orbits, yielding a Galactic population of at least several million. 相似文献
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