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Searching for Millisecond Pulsars: Surveys, Techniques and Prospects [PDF]

, 2013
Searches for millisecond pulsars (which we here loosely define as those with periods $
Lorimer, D. R., Lynch, R. S, Stovall, K.
core   +3 more sources

Millisecond Pulsars [PDF]

Highlights of Astronomy, 1989
AbstractMillisecond pulsars are intrinsically interesting because they illustrate some of the most extreme physical conditions to be found anywhere in the Universe, and because their evolution exhibits several stages of great drama. It had been widely believed for several years that spin-up of an old neutron star by accretion from a close stellar ...
openaire   +1 more source

Pulsars Cannot Account for the Inner Galaxy's GeV Excess [PDF]

, 2013
Using data from the Fermi Gamma-Ray Space Telescope, a spatially extended component of gamma rays has been identified from the direction of the Galactic Center, peaking at energies of ~2-3 GeV.
Cholis, Ilias, Hooper, Dan, Linden, Tim, Siegal-Gaskins, Jennifer, Slatyer, Tracy   +4 more
core   +2 more sources

Effect of low energy availability during three consecutive days of endurance training on iron metabolism in male long distance runners

Physiological Reports, Volume 8, Issue 12, June 2020., 2020
Three consecutive days of endurance training under low energy availability (LEA) decreased the muscle glycogen content and increased the serum hepcidin level in well‐trained male long distance runners. These results suggest that LEA is associated with a risk of exercise‐induced iron deficiency by an elevated hepcidin level in endurance athletes ...
Aya Ishibashi, Chihiro Kojima, Yoko Tanabe, Kaito Iwayama, Tsutomu Hiroyama, Toshiki Tsuji, Akiko Kamei, Kazushige Goto, Hideyuki Takahashi   +8 more
wiley   +1 more source

The characteristics of millisecond pulsar emission: I. Spectra, pulse shapes and the beaming fraction

, 1998
We have monitored a large sample of millisecond pulsars using the 100-m Effelsberg radio telescope in order to compare their radio emission properties to the slowly rotating population.
Alexander Wolszczan, Axel Jessner, Backer D. C., Bell J. F., Biggs J. D., Clifton T. R., D'Amico N., Doroshenko O. V., Duncan R. Lorimer, Fernando Camilo, Geppert U., Gil J. A., Gil J. A., Gil J. A., Jahan Miri M., Johnston S., Kanbach G., Kijak J., Kiriaki M. Xilouris, Kramer M., Kramer M., Lorimer D. R., Lorimer D. R., Lyne A. G., Malofeev V. M., Manchester R. N., Matese J. J., Michael Kramer, Narayan R., Nicastro L., Oleg Doroshenko, Ott M., Radhakrishnan V., Richard Wielebinski, Seiradakis J. H., Shklovskii I. S., Srinivasan G., Van den Heuvel E. P. J., von Hoensbroech A., von Hoensbroech A., Xilouris K. M.   +40 more
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Discovery of three new millisecond pulsars in Terzan 5 [PDF]

, 2018
We report on the discovery of three new millisecond pulsars (namely J1748-2446aj, J1748-2446ak and J1748-2446al) in the inner regions of the dense stellar system Terzan 5.
Cadelano, M., Ferraro, F. R., Freire, P. C. C., Hessels, J. W. T., Lanzoni, B., Pallanca, C., Ransom, S. M., Stairs, I. H.   +7 more
core   +2 more sources

Millisecond Pulsar Surveys [PDF]

Symposium - International Astronomical Union, 1987
In 1982 a new class of pulsars was defined by the discovery of a star with a millisecond rotation period, 1.6 ms. In the past 3.5 years two additional pulsars with millisecond periods have been discovered. The rapid spin of these pulsars is attributed to mass transfer in a low-mass binary progenitor system.
openaire   +1 more source

Millisecond Pulsar Surveys [PDF]

International Astronomical Union Colloquium, 1996
Abstract There are now more than 30 millisecond pulsars known to be associated with the Galactic disk. The majority of these have been discovered in just the last few years as the result of large-scale all-sky surveys. The properties of the population vary tremendously.
openaire   +1 more source

The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. V. Localization of Two Millisecond Pulsars

The Astrophysical Journal, 2023
The timing follow-up of newly discovered millisecond pulsars (MSPs) is hindered by the larger positional uncertainty (a few tens of arcminutes) associated with the discovery.
Shyam S. Sharma, Jayanta Roy, Sanjay Kudale, Bhaswati Bhattacharyya, Arpit K. Behera, Shubham Singh   +5 more
doaj   +1 more source

The Spin Distribution of Millisecond X-ray Pulsars

, 2008
The spin frequency distribution of accreting millisecond X-ray pulsars cuts off sharply above 730 Hz, well below the breakup spin rate for most neutron star equations of state. I review several different ideas for explaining this cutoff.
Alessandro Patruno, D. Chakrabarty, Diego Altamirano, Manuel Linares, Nanda Rea, Nathalie Degenaar, Paolo Soleri, Piergiorgio Casella, Rudy Wijnands   +8 more
core   +1 more source