Zobrazeno 1 - 10
of 10
pro vyhledávání: '"D. J. Hegyi"'
Publikováno v:
Annals of the New York Academy of Sciences. 262:404-408
Calculations for the maximum mass of a nonrotating neutron star are given. Results are compared with other neutron star masses. 13 references. (BJG)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bbc046827cf443f7dd99798b9eb7e368
https://doi.org/10.1111/j.1749-6632.1975.tb31457.x
https://doi.org/10.1111/j.1749-6632.1975.tb31457.x
Publikováno v:
Physical Review Letters. 28:1541-1544
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fc88fef23040c0cbb0d1750afa871949
https://doi.org/10.1103/physrevlett.28.1541
https://doi.org/10.1103/physrevlett.28.1541
Autor:
D. J. Hegyi
Speckle interferometry has been carried out during the last year with a charge-coupled device (CCD) imaging system. The emphasis of this project has been to minimize all systematic differences that arise between the images of stars in a binary star s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8b7df62ec2074d0b512d6ccdf54b59fa
https://doi.org/10.21236/ada139297
https://doi.org/10.21236/ada139297
Publikováno v:
The Astrophysical Journal. 190:543
The R(2) line of the 3874 A band of interstellar CN toward zeta Oph was measured. An equivalent width of 0.120 mA implying an R(2)-R(1) rotational temperature of about 3.1 K was observed. Taking into account also earlier observations, it is found tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1e771f6091143a3470b00e18c3c50723
https://doi.org/10.1086/152908
https://doi.org/10.1086/152908
Autor:
G. L. Gerber, D. J. Hegyi
Publikováno v:
The Astrophysical Journal. 218:L7
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::75dafcb65f1f10a3dfa34677d07b3be4
https://doi.org/10.1086/182565
https://doi.org/10.1086/182565
Publikováno v:
The Astrophysical Journal. 190:L81
Results of a search for D alpha emission near the bright H alpha line in Orion. The observations revealed a high-velocity H alpha feature near -60 km/sec, whose intensity varied across the nebula, ranging from 0.005 to 0.005 relative to H alpha; anot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af1f3b70c6e16ec7faab9a243b270ffd
https://doi.org/10.1086/181511
https://doi.org/10.1086/181511
Autor:
D. J. Hegyi, Adam Burrows
Publikováno v:
The Astronomical Journal. 85:1421
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e80c945cb1e2f8695a2b7a8ad50b6841
https://doi.org/10.1086/112816
https://doi.org/10.1086/112816
Autor:
R. P. Geroch, D. J. Hegyi
Publikováno v:
Nature. 215:501-501
WE offer a new approach to an old1 question: “Given a material medium with its equation of state, what conditions must be satisfied by that equation of state if the existence of such matter is to be consistent with the principles of special relativ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::34c5dd6ff47f2a41d99c48e66e2a7bb9
https://doi.org/10.1038/215501a0
https://doi.org/10.1038/215501a0
Autor:
D. R. Curott, D. J. Hegyi
Publikováno v:
Applied Optics. 10:651
A photoelectric stellar image analyzer has been constructed to measure the separation of close binary stars (about 1 sec of arc separation). Data are collected by coherent superposition of thousands of images thereby reducing the effects of the atmos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7de84db1a69a20932a6e049e326ade4
https://doi.org/10.1364/ao.10.000651
https://doi.org/10.1364/ao.10.000651
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