Showing 521 - 540 results of 925 for search '"effective temperature"', query time: 0.49s Refine Results
  1. 521

    An injectable hyperthermic nanofiber mesh with switchable drug release to stimulate chemotherapy potency by Lili Chen, Nanami Fujisawa, Nanami Fujisawa, Masato Takanohashi, Mitsuhiro Ebara, Mitsuhiro Ebara, Mitsuhiro Ebara

    Published 2022-11-01
    “…In heat-generation measurements, the mesh achieved an effective temperature of mild hyperthermia (41–43°C) within 5 min of exposure to alternating magnetic field (AMF) irradiation. …”
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    Article
  2. 522

    Phase Transformations Caused by Heat Treatment and High-Pressure Torsion in TiZrHfMoCrCo Alloy by Alena S. Gornakova, Boris B. Straumal, Alexander I. Tyurin, Natalia S. Afonikova, Alexander V. Druzhinin, Gregory S. Davdian, Askar R. Kilmametov

    Published 2023-02-01
    “…This state is similar to the state after annealing at high effective temperature <i>T</i><sub>eff</sub>. The additional annealing at 1000 °C after HPT returns the phase composition back to the state similar to that of the as-cast alloy after annealing at 1000 °C. …”
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    Article
  3. 523

    Volcanic Anomalies Monitoring System (VOLCANOMS), a Low-Cost Volcanic Monitoring System Based on Landsat Images by Susana Layana, Felipe Aguilera, Germán Rojo, Álvaro Vergara, Pablo Salazar, Juan Quispe, Pablo Urra, Diego Urrutia

    Published 2020-05-01
    “…VOLCANOMS allows researchers to calculate several thermal parameters, such as thermal radiance, effective temperature, anomaly area, radiative, gas, convective, and total heat, and mass fluxes. …”
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    Article
  4. 524

    3D Radiation-hydrodynamic Simulations Resolving Interior of Rapidly Accreting Primordial Protostar by Kazutaka Kimura, Takashi Hosokawa, Kazuyuki Sugimura, Hajime Fukushima

    Published 2023-01-01
    “…We demonstrate that, in both cases, a swollen protostar whose radius is 100–1000 R _⊙ appears, as predicted by the stellar evolution calculations. Its effective temperature remains a few thousand Kelvin, and the radiative feedback by ionizing photons is too weak to disturb the accretion flow up to the epoch examined in this work. …”
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    Article
  5. 525

    Climate chamber investigation of the effect of indoor thermal histories on thermal adaptation in different seasons by Yuxin Wu, Angchen Jiang, Hong Liu, Baizhan Li, Risto Kosonen

    Published 2024-06-01
    “…However, the TSV of AC subjects were much lower than that of NV subjects in the same standard effective temperature and skin temperature in a cold environment in winter. …”
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    Article
  6. 526

    A Comprehensive Study on Outdoor Thermal Comfort in Arid Urban Environments through Microclimatic Analysis of Urban Density by Alaa Eddine Bacha, Atef Ahriz, Mohammad Alshenaifi, Sultan Alfraidi, Emad Noaime, Badr Alsolami, Aritra Ghosh, Soumia Bouzaher, Lambros T. Doulos, Abdelhakim Mesloub

    Published 2024-03-01
    “…We captured air temperature, humidity, and wind velocity to enable thermal comfort assessment via the Effective Temperature (ET) and Equivalent Temperature (TEK) stress indices. …”
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    Article
  7. 527

    The SkyMapper DR1.1 search for extremely metal-poor stars by Da Costa, GS, Bessell, MS, Mackey, AD, Nordlander, T, Asplund, M, Casey, AR, Frebel, A, Lind, K, Marino, AF, Murphy, SJ, Norris, JE, Schmidt, BP, Yong, D

    Published 2021
    “…In particular, we outline our photometric selection procedures and describe the low-resolution (R ≈ 3000) spectroscopic follow-up observations that are used to provide estimates of effective temperature, surface gravity, and metallicity ([Fe/H]) for the candidates. …”
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    Article
  8. 528

    The SkyMapper DR1.1 search for extremely metal-poor stars by Da Costa, GS, Bessell, MS, Mackey, AD, Nordlander, T, Asplund, M, Casey, AR, Frebel, Anna L., Lind, K, Marino, AF, Murphy, SJ, Norris, JE, Schmidt, BP, Yong, D

    Published 2022
    “…In particular, we outline our photometric selection procedures and describe the low-resolution (R ≈ 3000) spectroscopic follow-up observations that are used to provide estimates of effective temperature, surface gravity, and metallicity ([Fe/H]) for the candidates. …”
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    Article
  9. 529

    Thermally regenerative electrochemically cycled flow batteries with pH neutral electrolytes for harvesting low-grade heat by Qian, Xin, Shin, Jungwoo, Tu, Yaodong, Zhang, James Han, Chen, Gang

    Published 2021
    “…Electrochemical methods for harvesting low-grade heat have aroused research interest in recent years due to the relatively high effective temperature coefficient of the electrolytes (>1 mV K⁻¹) compared with the thermopower of traditional thermoelectric devices. …”
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    Article
  10. 530

    Disentangling the Planet from the Star in Late-Type M Dwarfs: A Case Study of TRAPPIST-1g by Wakeford, HR, Lewis, NK, Fowler, J, Bruno, G, Wilson, TJ, Moran, SE, Valenti, J, Batalha, NE, Filippazzo, J, Bourrier, V, Hörst, SM, Lederer, SM, de Wit, J

    Published 2022
    “…We find that TRAPPIST-1 is a 0.08 M ∗, 0.117 R ∗, M8V star with a photospheric effective temperature of 2400 K, with ∼35% 3000 K spot coverage and a very small fraction, <3%, of ∼5800 K hot spot. …”
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    Article
  11. 531

    KELT-9 b’s Asymmetric TESS Transit Caused by Rapid Stellar Rotation and Spin–Orbit Misalignment by Ahlers, John P, Johnson, Marshall C, Stassun, Keivan G, Colón, Knicole D, Barnes, Jason W, Stevens, Daniel J, Beatty, Thomas, Gaudi, B Scott, Collins, Karen A, Rodriguez, Joseph E, Ricker, George, Vanderspek, Roland, Latham, David, Seager, Sara, Winn, Joshua, Jenkins, Jon M, Caldwell, Douglas A, Goeke, Robert F, Osborn, Hugh P, Paegert, Martin, Rowden, Pam, Tenenbaum, Peter

    Published 2022
    “…We also apply a gravity-darkening correction to the spectral energy distribution model from Gaudi et al. and find that accounting for rapid rotation gives a better fit to available spectroscopy and yields a more reliable estimate for the star's polar effective temperature.…”
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    Article
  12. 532

    Discovery of a young low-mass brown dwarf transiting a fast-rotating F-type star by the Galactic Plane eXoplanet (GPX) survey by Burdanov, Artem, Ricker, George R, Vanderspek, Roland K, Seager, Sara

    Published 2022
    “…We use the isochrone placement algorithm to characterize the host star, which has effective temperature 7000 ± 200 K, mass 1.68 ± 0.10 $\mathrm{\it M}_\odot$, radius 1.56 ± 0.10 $\mathrm{\it R}_\odot$, and approximate age $0.27_{-0.15}^{+0.09}$ Gyr. …”
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    Article
  13. 533
  14. 534
  15. 535

    THE INITIAL MASS FUNCTION OF THE ORION NEBULA CLUSTER ACROSS THE H-BURNING LIMIT by Da Rio, N., Robberto, M., Hillenbrand, L. A., Henning, T., Stassun, Keivan

    Published 2015
    “…We develop and exploit a technique to determine stellar effective temperatures from optical colors, nearly doubling the previously available number of objects with effective temperature determinations in this benchmark cluster. …”
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    Article
  16. 536

    KOI 1224: A FOURTH BLOATED HOT WHITE DWARF COMPANION FOUND WITH KEPLER by Breton, Rene P., van Kerkwijk, M. H., Carter, Joshua Adam, Rappaport, Saul A

    Published 2015
    “…The ingredients that are used in the analysis are the Kepler binary light curve, including the detection of the Doppler boosting effect; the NUV and FUV fluxes from the GALEX images of this object; an estimate of the spectral type of the F-star companion; and evolutionary models of the companion designed to match its effective temperature and mean density. The light curve is modeled with a new code named Icarus which we describe in detail. …”
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    Article
  17. 537

    Machine Learning based Prediction of Thermal Comfort in Buildings of Equatorial Singapore by Chaudhuri, Tanaya, Soh, Yeng Chai, Li, Hua, Xie, Lihua

    Published 2017
    “…Age, gender, and outdoor effective temperature, which are not included in the PMV model, are found to be important factors for thermal comfort. …”
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    Conference Paper
  18. 538

    The photospheric abundances of active binaries - 1. Detailed analysis of HD 113816 (IS Vir) and HD 119285 (V851 Cen) by Katz, D, Favata, F, Aigrain, S, Micela, G

    Published 2003
    “…It is shown that the V - I photometric index gives, on a broader sample of stars, significantly cooler estimates of the effective temperature than the B - v index. All approaches give results in good agreement with each other, except the V - 1 based method. …”
    Journal article
  19. 539

    Isothermal dust models of Herschel-ATLAS star galaxies by Smith, D, Hardcastle, M, Jarvis, M, Maddox, S, Dunne, L, Bonfield, D, Eales, S, Serjeant, S, Thompson, M, Baes, M, Clements, D, Cooray, A, De Zotti, G, Gonzalez-Nuevo, J, van der Werf, P, Virdee, J, Bourne, N, Dariush, A, Hopwood, R, Ibar, E, Valiante, E

    Published 2013
    “…This is true even for galaxies with the most robust statistical detections in our sample, making the results of such fitting difficult to interpret.We apply a method to determine the best-fitting global values of isothermal effective temperature and emissivity index for z &lt; 0.5 galaxies in H-ATLAS, deriving Teff = 22.3 ± 0.1K and β = 1.98 ± 0.02 (or Teff = 23.5 ± 0.1K and β = 1.82 ± 0.02 if we attempt to correct for bias by assuming that Teff and βeff are independent and normally distributed). …”
    Journal article
  20. 540

    Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey by Pinfield, D, Burningham, B, Tamura, M, Leggett, S, Lodieu, N, Lucas, P, Mortlock, D, Warren, S, Homeier, D, Ishii, M, Deacon, N, McMahon, R, Hewett, P, Osori, M, Martin, E, Jones, H, Venemans, B, Day-Jones, A, Dobbie, P, Folkes, S, Dye, S, Allard, F, Baraffe, I, Barrado y Navascu, D, Casewell, S

    Published 2008
    “…The colours of the full sample of LAS T dwarfs show a possible trend to bluer Y - J with decreasing effective temperature, and some interesting colour changes in J - H and z - J (deserving further investigation) beyond T8. …”
    Journal article