Results 11 to 20 of about 1,171,364 (102)

Star wreck [PDF]

Physics Letters B, 1998
9 pages; references ...
Kusenko, Alexander, Shaposhnikov, Mikhail, Tinyakov, P. G., Tkachev, Igor I.   +3 more
openaire   +2 more sources

The VLT-FLAMES Tarantula Survey IV: Candidates for isolated high-mass star formation in 30 Doradus [PDF]

, 2012
Whether massive stars can occasionally form in relative isolation or if they require a large cluster of lower-mass stars around them is a key test in the differentiation of star formation theories as well as how the initial mass function of stars is ...
A. de Koter, Alves, André, Baade, Banerjee, Bastian, Bastian, Bastian, Bastian, Bergin, Bertin, Bestenlehner, Bonnell, Bonnell, Brandner, Bressert, Brott, C. J. Evans, Campbell, Chu, Cioni, Comeron, Danziger, de Koter, De Marchi, de Wit, de Wit, E. Bressert, Efremov, Elmegreen, Evans, G. Gräfener, Gieles, Girichidis, Gruendl, Gvaramadze, Gvaramadze, Gvaramadze, H. Sana, Huthoff, J. M. Bestenlehner, J. M. D. Kruijssen, J. Maíz Apellániz, J. S. Vink, King, Kissler-Patig, Kraus, Kroupa, Kruijssen, Kruijssen, Krumholz, Lamb, Lazendic, Lejeune, M. Cantiello, M. Gieles, Maeder, Martins, Maschberger, Maschberger, Massey, Massey, Maíz-Apellániz, McKee, Meixner, Meixner, Melnick, Meynet, Moffat, Molinari, N. Bastian, Oey, P. A. Crowther, Parker, Parker, Pasquini, Peimbert, Pellegrini, Popescu, Portegies Zwart, R. J. Parker, S. N. Longmore, S. P. Goodwin, Sana, Scheepmaker, Schild, Selier, Selman, Selman, Smith, Tenorio-Tagle, V. Hénault-Brunet, van Buren, W. D. Taylor, Wadadekar, Walborn, Walborn, Walborn, Walborn, Walborn, Walborn, Weidner, Weidner, Weidner, Werchan, Wheelwright, Yorke   +106 more
core   +3 more sources

Incidence and survival of remnant disks around main-sequence stars [PDF]

, 2000
We present photometric ISO 60 and 170um measurements, complemented by some IRAS data at 60um, of a sample of 84 nearby main-sequence stars of spectral class A, F, G and K in order to determine the incidence of dust disks around such main-sequence stars ...
A. Salama, Artymowicz, Artymowicz, Ash, Aumann, Aumann, Burns, Butler, C. Dominik, Chini, Chyba, Dent, Dominik, Draine, Ferlet, H. J. Habing, Habing, Habing, Hobbs, Holland, Jayawardhana, Johnson, Jourdain de Muizon, K. Leech, Kamp, Kessler, Kunzli, L. Metcalfe, Lachaume, Lemke, Liseau, M. F. Kessler, M. Jourdain de Muizon, , Mannings, N. Trams, Natta, Neukum, P. Bouchet, Plets, R. J. Laureijs, R. Siebenmorgen, Sargent, Smith, Soderblom, Trilling, Walker, Waters, Weissman, Zahnle, Zuckerman, Ábrahám   +50 more
core   +3 more sources

Moduli stars [PDF]

Journal of High Energy Physics, 2018
AbstractWe explore the possibility that (Bose-Einstein) condensation of scalar fields from string compactifications can lead to long-lived compact objects. Depending on the type of scalar fields we find different realisations of star-like and solitonic objects.
Krippendorf, Sven, Muia, Francesco, Quevedo, Fernando   +2 more
openaire   +4 more sources

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

J-type Carbon Stars in the Large Magellanic Cloud

, 2003
A sample of 1497 carbon stars in the Large Magellanic Cloud has been observed in the red part of the spectrum with the 2dF facility on the AAT. Of these, 156 have been identified as J-type (i.e.
Abia, B. F. W. Croke, Bailey, Barnbaum, Barnbaum, Bergeat, Bessell, Blanco, Cannon, Cioni, Cowley, Crabtree, D. H. Morgan, D. Hatzidimitriou, Dapergolas, Feast, Gordon, Hartwick, Hatzidimitriou, Keenan, Kontizas, Kontizas, Kontizas, Kontizas, Lambert, Lewis, Lloyd Evans, Lorenz-Martins, Marenin, Morgan, Morgan, R. D. Cannon, Richer, Richer, Skrutskie, Suntzeff, Vanture, Westerlund, Westerlund, Westerlund, Westerlund   +40 more
core   +1 more source

Stars, Anti-Stars, Anti-Star-Stars

Persona Studies
The phenomenon of stars and celebrities in media cultures – and especially in popular music cultures – seems to be omnipresent. At the same time, there is an astounding lack of analysis and research on these media personalities and personas, and international celebrity studies only recently a developing new field. Similarly, these kinds of observations
openaire   +3 more sources

Extended shells around B[e] stars - implications for B[e] star evolution [PDF]

, 2008
Aims. The position of B[e] stars in the upper left part of the Hertzsprung-Russell diagram creates a quandary. Are these stars young stars evolving onto the main sequence or old stars that are evolving off of it? Spectral characteristics suggest that B[e]
Marston, M. P., McCollum, B.
core  

The physics and chemistry of circumstellar envelopes of S-stars on the AGB

, 2007
The S-stars have been suggested to be a brief transitional phase as stars evolve from oxygen-rich M-type stars into carbon stars, through the dredge up of carbon from He-shell burning.
Olofsson, H., Ramstedt, S., Schoeier, F. L.   +2 more
core   +1 more source

Rotation and Macroturbulence in Metal-poor Field Red Giant and Red Horizontal Branch Stars [PDF]

, 2007
We report the results for rotational velocities, Vrot sin i, and macroturbulence dispersion, zeta(RT), for 12 metal-poor field red giant branch stars and 7 metal-poor field red horizontal branch stars.
Bruce W. Carney, Carney B. W., Carney B. W., David F. Gray, David W. Latham, David Yong, Dupree A. K., Gray D. F., John B. Laird, Kinman T., Massarotti A., Nadine Manset, Rachel Zelman   +12 more
core   +3 more sources