Zobrazeno 1 - 10
of 257
pro vyhledávání: '"P. Crause"'
Publikováno v:
Resuscitation Plus, Vol 17, Iss , Pp 100543- (2024)
Background: The incidence of cardiovascular diseases, and with it out-of-hospital cardiac arrest (OHCA), is on the increase in low- to middle-income countries (LMICs), like South Africa. Interventions such as mass public cardiopulmonary resuscitation
Externí odkaz:
https://doaj.org/article/344c930f875447be8eb2e7f031982a83
Autor:
Saunders, Nicholas, Grunblatt, Samuel K., Huber, Daniel, Collins, Karen A., Jensen, Eric L. N., Vanderburg, Andrew, Brahm, Rafael, Jordán, Andrés, Espinoza, Néstor, Henning, Thomas, Hobson, Melissa J., Quinn, Samuel N., Zhou, George, Butler, R. Paul, Crause, Lisa, Kuhn, Rudi B., Mogotsi, K. Moses, Hellier, Coel, Angus, Ruth, Hattori, Soichiro, Chontos, Ashley, Ricker, George R., Jenkins, Jon M., Tenenbaum, Peter, Latham, David W., Seager, Sara, Vanderspek, Roland K., Winn, Joshua N., Stockdale, Chris, Cloutier, Ryan
While the population of confirmed exoplanets continues to grow, the sample of confirmed transiting planets around evolved stars is still limited. We present the discovery and confirmation of a hot Jupiter orbiting TOI-2184 (TIC 176956893), a massive
Externí odkaz:
http://arxiv.org/abs/2108.02294
Autor:
Shara, Michael M., Crawford, Steven M., Vanbeveren, Dany, Moffat, Anthony F. J., Zurek, David, Crause, Lisa
Some massive, merging black holes (BH) may be descendants of binary O stars. The evolution and mass transfer between these O stars determines the spins of their progeny BH. These will be measurable with future gravitational wave detectors, incentiviz
Externí odkaz:
http://arxiv.org/abs/2001.01012
Planetary Nebulae are the ionised ejected envelopes surrounding the remnant cores of dying stars. Theory predicts that main-sequence stars with one to about eight times the mass of our sun may eventually form planetary nebulae. Until now no example h
Externí odkaz:
http://arxiv.org/abs/1906.10556
Autor:
Gomel, Roy, Shahaf, Sahar, Mazeh, Tsevi, Faigler, Simchon, Crause, Lisa A., Sefako, Ramotholo, Segransan, Damien, Maxted, Pierre F. L., Soszyński, Igor
We report here on a detailed study of a c-type RR Lyrae variable (RRc variable), SB 796, serendipitously discovered in a search of the WASP public data for stars that display large photometric periodic modulation. SB 796 displays a period of $P = 0.2
Externí odkaz:
http://arxiv.org/abs/1810.09501
The MeerKAT radio telescope array, the Large Synoptic Survey Telescope (LSST), and eventually the Square Kilometer Array (SKA) will usher in a remarkable new era in astronomy, with thousands of transients being discovered and transmitted to the astro
Externí odkaz:
http://arxiv.org/abs/1808.00138
Autor:
Shara, Michael M., Ilkiewicz, Krystian, Mikolajewska, Joanna, Pagnotta, Ashley, Bode, Michael F., Crause, Lisa A., Drozd, Katarzyna, Faherty, Jacqueline K., Fuentes-Morales, Irma, Grindlay, Jonathan E., Moffat, Anthony F. J., Schmidtobreick, Linda, Stephenson, F. Richard, Tappert, Claus, Zurek, David
Here we report the recovery of the binary underlying the classical nova of 11 March 1437 A.D. whose age is independently confirmed by proper motion-dating, and show that in the 20th century it exhibits dwarf nova eruptions. The four oldest recovered
Externí odkaz:
http://arxiv.org/abs/1704.00086
Autor:
Macfarlane, S. A., Woudt, P. A., Groot, P. J., Ramsay, G., Toma, R., Motsoaledi, M., Crause, L. A., Gilbank, D. G., O'Donoghue, D., Potter, S. B., Sickafoose, A. A., van Gend, C., Worters, H. L.
We present photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey: a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane. We have used fast photometry on the SAAO 1.0
Externí odkaz:
http://arxiv.org/abs/1610.05687
The spin rates of O stars in WR + O binaries. I. Motivation, methodology and first results from SALT
Autor:
Shara, Michael M., Crawford, Steven M., Vanbeveren, Dany, Moffat, Anthony F. J., Zurek, David, Crause, Lisa
The black holes (BH) in merging BH-BH binaries are likely progeny of binary O stars. Their properties, including their spins, will be strongly influenced by the evolution of their progenitor O stars. The remarkable observation that many single O star
Externí odkaz:
http://arxiv.org/abs/1511.00046
Autor:
Déborah Hoffmam Crause, Edney Leandro da Vitória, Luis Felipe Oliveira Ribeiro, Francisco de Assis Ferreira, Yubin Lan, Pengchao Chen
Publikováno v:
Agronomy, Vol 13, Iss 6, p 1506 (2023)
The yield of coffee plants depends on several factors, and the leaf nutrition is one of the most important. The form of application of leaf fertilizers used is expensive considering the application efficacy and the efficacy of adherence and absorptio
Externí odkaz:
https://doaj.org/article/9426946007e3400bb003e0b277f006ed