1,727,499 research outputs found
Cim del Pedraforca (2498 m.)
No full textBoItinerari: Saldes (1213 m.) - Cim del Pedraforca (2498 m.) Salde
2498. Theodoricus de Apoldia
No full text2498. Theodoricus de Apoldia. In: Molinier Auguste. Les Sources de l'histoire de France - Des origines aux guerres d'Italie (1494). III. Les Capétiens, 1180-1328. Paris : A. Picard et fils, 1903. p. 78
Baseline characteristics of 2498 participating ACS patients.
No full textBaseline characteristics of 2498 participating ACS patients.</p
2498. Theodoricus de Apoldia
No full text2498. Theodoricus de Apoldia. In: Molinier Auguste. Les Sources de l'histoire de France - Des origines aux guerres d'Italie (1494). III. Les Capétiens, 1180-1328. Paris : A. Picard et fils, 1903. p. 78
Demographic profile of the study participants by region (n = 2498).
No full textDemographic profile of the study participants by region (n = 2498).</p
Congressional Record S. 2498 - Montana Railroad Mergers and Service Curtailment
Get PDFCongressional Record S. 2498 - Montana Railroad Mergers and Service Curtailmen
Walker, Josephine, 1864-1944 (SC 2498)
Get PDFFinding aid only for Manuscripts Small Collection 2498. Diary kept by Josephine Walker, Columbia, Adair County, Kentucky from 4 November 1891 to 10 October 1893. She records the weather, visits, illnesses, local births and deaths, and everyday household and farm activities such as food preparation,quilting, sewing, and her piano playing. Local family names mentioned include Traylor, Diddle, Flowers, Atkins and Murrell
TOI-2498 b: A hot bloated super-Neptune within the Neptune desert
Get PDFWe present the discovery and confirmation of a transiting hot, bloated
Super-Neptune using photometry from TESS and LCOGT and radial velocity
measurements from HARPS. The host star TOI-2498 is a V = 11.2, G-type
(T = 5905 12K) solar-like star with a mass of 1.12 0.02
M and a radius of 1.26 0.04 R. The planet, TOI-2498
b, orbits the star with a period of 3.7 days, has a radius of 6.1 0.3
R, and a mass of 35 4 M. This results in a density
of 0.86 0.25 g cm. TOI-2498 b resides on the edge of the Neptune
desert; a region of mass-period parameter space in which there appears to be a
dearth of planets. Therefore TOI-2498 b is an interesting case to study to
further understand the origins and boundaries of the Neptune desert. Through
modelling the evaporation history, we determine that over its 3.6 Gyr
lifespan, TOI-2498 b has likely reduced from a Saturn sized planet to its
current radius through photoevaporation. Moreover, TOI-2498 b is a potential
candidate for future atmospheric studies searching for species like water or
sodium in the optical using high-resolution, and for carbon based molecules in
the infra-red using JWST.Comment: 13 pages, 11 figures, accepted for publication in MNRA
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