Results 21 to 30 of about 1,401,162 (283)

RXJ1856.5-3754 and RXJ0720.4-3125 are P-Stars

, 2004
P-stars are a new class of compact stars made of up and down quarks in $\beta$-equilibrium with electrons in a chromomagnetic condensate. P-stars are able to account for compact stars with $R \lesssim 6 Km$, as well as stars comparable to canonical ...
Cea, Paolo
core   +1 more source

Checking the possibility of determining the relative orbits of stars rotating around the center body of the Galaxy

Open Astronomy, 2022
The results of observations of selected stars orbiting the central body of our Galaxy, which, according to the latest data, has a mass of about 4 million of solar mass, are considered.
Shakht Natalia A., Izmailov Igor S., Gorshanov Denis L.   +2 more
doaj   +1 more source

How to identify a Strange Star [PDF]

, 1998
Contrary to young neutron stars, young strange stars are not subject to the r-mode instability which slows rapidly rotating, hot neutron stars to rotation periods near 10 ms via gravitational wave emission.
A. Goyal, C. Alcock, C. Cutler, C. J. Pethick, C. Schaab, E. Witten, H. Heiselberg, H. Heiselberg, H. Heiselberg, J. L. Friedman, J. L. Zdunik, J. M. Lattimer, J. Madsen, J. Madsen, Jes Madsen, L. Lindblom, M. Colpi, N. Andersson, N. K. Glendenning, P. Haensel, Q. D. Wang, R. F. Sawyer, Z. Dai   +22 more
core   +2 more sources

THE DETERMINATION OF PERIODS AND THE DEFINITION OF VARIABILITY TYPE OF NEW VARIABLE STAR IRAS 17583+5150

Odessa Astronomical Publications, 2017
The measurements of brightness of the star IRAS 17583+5150 discovered using the Odessa observatory negatives are discussed in the article. The proposed types of these stars are IRAS 17583+5150 -- type SRB (SRC).
A. P. Solonovich, I. S. Bryukhanov
doaj   +1 more source

Properties of massive stars in four clusters of the VVV survey

, 2015
The evolution of massive stars is only partly understood. Observational constraints can be obtained from the study of massive stars located in young massive clusters.
Borissova, J., Bouret, J. -C., Chené, A. -N., Hervé, A., Martins, F.   +4 more
core   +3 more sources

Moving in the Dark: Enlightening the Spatial Population Ecology of European Cave Salamanders

Population Ecology, EarlyView.
We assessed individual interactions, movement ecology and activity patterns of a subterranean population of Speleomantes strinatii, applying spatial capture–recapture modeling to a photographic dataset of 104 individuals. ABSTRACT Space use and movement are fundamental aspects of organisms' ecology, mirroring individual fitness, behavior, and life ...
Giacomo Rosa, Andrea Costa, Sebastiano Salvidio   +2 more
wiley   +1 more source

Catalog of Galactic Beta Cephei Stars

, 2005
We present an extensive and up-to-date catalog of Galactic Beta Cephei stars. This catalog is intended to give a comprehensive overview of observational characteristics of all known Beta Cephei stars.
Aerts C., Aerts C., Aerts C., Aerts C., Aerts C., Aerts C., Aerts C., Aerts C., Anamarija Stankov, Antokhina E. A., Ausseloos M., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Balona L. A., Batten A. H., Bernacca P. L., Breger M., Catalano F. A., Chapellier E., Chapellier E., Chapellier E., Cote J., Cousins A. W. J., Cugier H., Cugier H., Cuypers J., Cuypers J., Dachs J., Dachs J., De Cat P., De Mey K., De Mey K., De Ridder J., Delgado A. J., Delgado A. J., Delgado A. J., Deupree R., Duflot M., Dufton P. L., Dziembowski W., Dziembowski W. A., Dziembowski W. A., Elst E. W., Elst E. W., Engelbrecht C. A., Feast M. W., Feast M. W., Frost E. B., Frost E. B., Garrido R., Gautschy A., Gerald Handler, Gomez-Forrellad J. M., Goosens M., Guthnick P., Hadrava P., Haefner R., Hambly N. C., Handler G., Harmanec P., Harmanec P., Henroteau F., Henroteau F., Heynderickx D., Heynderickx D., Hill G., Hill P. W., Hill P. W., Hill P. W., Hoag A. A., Holmgren D., Irvine N. J., Jakate S. M., Jakate S. M., Jakate S. M., Janik J., Jarzebowski T., Jaschek M., Jerzykiewicz M., Jerzykiewicz M., Jerzykiewicz M., Jerzykiewicz M., Jerzykiewicz M., Jerzykiewicz M., Jerzykiewicz M., Jerzykiewicz M., Jones D. H. P., Kazarovets A. V., Khokhlova V. L., Kilkenny D., Kilkenny D., Kilkenny D., Koen C., Kolaczkowski Z., Krisciunas K., Krisciunas K., Krzesinski J., Krzesinski J., Kubiak M., Kubiak M., Le Contel J.-M., Lehmann H., Leone F., Lesh J. R., Lester J. B., Levato H., Lloyd C., Lomb N. R., Lomb N. R., Lynds C. R., Lynds C. R., Maciejewski G., Mahra H. S., Mathias P., Mathias P., Mathias P., Matthews J. M., Matthews J. M., McNamara B. J., Moon T. T., Moskalik P., Napiwotzki R., Paardekooper S. J., Pamyatnykh A. A., Pamyatnykh A. A., Pamyatnykh A. A., Pedersen H., Percy J. R., Percy J. R., Percy J. R., Percy J. R., Pietrzynski G., Pigulski A., Pigulski A., Pigulski A., Plaskett J. S., Renson P., Renson P., Robb R. M., Saxena B. K., Schrijvers C., Schrijvers C., Shaw J. S., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Shobbrook R. R., Smith M. A., Smith M. A., Smith M. A., Stankov A., Stebbins J., Steele I. A., Sterken C., Sterken C., Sterken C., Sterken C., Sterken C., Sterken C., Sterken C., Stickland D. J., Struve O., Struve O., Telting J. H., Telting J. H., Telting J. H., Thoul A., Tian B., Uytterhoeven K., Uytterhoeven K., Uytterhoeven K., Valtier J. C., Van Hoof A., Van Hoof A., Van Hoof A., Vander Linden D., Vander Linden D., Vidal N. V., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Waelkens C., Walker M. F., Young R. K.   +211 more
core   +2 more sources

Observational Constraints on First-Star Nucleosynthesis. I. Evidence for Multiple Progenitors of CEMP-no Stars [PDF]

, 2016
We investigate anew the distribution of absolute carbon abundance, $A$(C) $= \log\,\epsilon $(C), for carbon-enhanced metal-poor (CEMP) stars in the halo of the Milky Way, based on high-resolution spectroscopic data for a total sample of 305 CEMP stars ...
Beers, Timothy C., Carollo, Daniela, Hansen, Terese T., He, Siyu, Placco, Vinicius M., Rasmussen, Kaitlin C., Roederer, Ian U., Yoon, Jinmi, Zeanah, Jeff   +8 more
core   +2 more sources

Infection Models for Pine Wilt Disease on the Basis of Vector Behaviors

Population Ecology, EarlyView.
Infection models for pine wilt disease without vector density were built to estimate the transmission coefficient of the pathogenic nematode. The models successfully simulated the annual change in the density of infected trees for four pine stands. ABSTRACT Pine wilt disease is caused by the pinewood nematode (Bursaphelenchus xylophilus Steiner et ...
Katsumi Togashi
wiley   +1 more source

Comparison of five video-assisted intubation devices by novice and expert laryngoscopists for use in the aeromedical evacuation environment

Military Medical Research, 2017
Background The critically ill or injured patient undergoing military medical evacuation may require emergent intubation. Intubation may be life-saving, but it carries risks.
Matthew C. Wallace, SSgt Tyler Britton, Robbie Meek, Sharon Walsh-Hart, Col Todd E. Carter, Steven J. Lisco   +5 more
doaj   +1 more source