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Books on the topic 'Pulsar observations'

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Author: Grafiati

Published: 4 June 2021

Last updated: 12 February 2022

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1

López Coto, Rubén. Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with MAGIC and Development of Trigger Systems for IACTs. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-44751-3.

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2

Frail, Dale A. A study of the diffuse interstellar medium through neutral hydrogen absorption observations toward pulsars. Toronto: University of Toronto, Dept. of Astronomy, 1989.

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3

EGRET observations of the Vela pulsar, PSR 0833-45. Garching, Germany: Max-Planck-Institut fur Extraterrestrische Physik, 1994.

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4

G, Kanbach, and United States. National Aeronautics and Space Administration., eds. EGRET observations of the Vela pulsar, PSR 0833-45. Garching, Germany: Max-Planck-Institut fur Extraterrestrische Physik, 1994.

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5

United States. National Aeronautics and Space Administration., ed. [ROSAT observations of the binary BE-star/radio pulsar PSR1259-6]: [semiannual technical report, 15 Jan. - 1 Aug. 1993]. [Washington, DC: National Aeronautics and Space Administration, 1993.

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6

[ROSAT observations of the binary BE-star/radio pulsar PSR1259-6]: [semiannual technical report, 15 Jan. - 1 Aug. 1993]. [Washington, DC: National Aeronautics and Space Administration, 1993.

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7

R, Cominsky Lynn, and United States. National Aeronautics and Space Administration., eds. ROSAT observations of the binary Be-star/radio pulsar PSR1259-63: Final technical report for NASA NAG 5-1684. [Washington, DC: National Aeronautics and Space Administration, 1994.

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8

ROSAT observations of the binary Be-star/radio pulsar PSR1259-63: Final technical report for NASA NAG 5-1684. [Washington, DC: National Aeronautics and Space Administration, 1994.

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9

Coto, Rubén López. Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with MAGIC and Development of Trigger Systems for IACTs. Springer, 2018.

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10

Maggiore, Michele. Neutron stars. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.003.0002.

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Observation of neutron stars as pulsars. Pulsar demography. Magnetars. GW emission from neutron stars. Normal modes of neuton stars. CFS instability; r-mode instability. GWs from the post-merger NS remnant. Ellipticity of deformed neutron stars.

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11

A, Prince Thomas, and United States. National Aeronautics and Space Administration., eds. Observations of accreting pulsars. [Washington, DC: National Aeronautics and Space Administration, 1994.

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12

Christopher, Martin, Marshall Herman L, and United States. National Aeronautics and Space Administration., eds. The Geminga pulsar: Soft X-Ray variability and an EUVE observation. [Washington, DC: National Aeronautics and Space Administration, 1996.

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13

Yang, Jingduan, and Daniel A. Monti. Evaluation of Human Energy. Oxford University Press, 2017. http://dx.doi.org/10.1093/med/9780190210052.003.0009.

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This chapter describes in detail how the human energetic status is evaluated through inquiry, observation, and palpation, including unique techniques such as tongue and pulse diagnosis. Diagnostic algorithms evaluating imbalances of the human energy system help readers to apply these techniques and utilize all the theories discussed in the previous chapters to effectively formulate a diagnosis, which is the key to successful treatment. The chapter also discusses how the energetic evaluation should and can be an integral part of a medical diagnosis. It also discusses other unique observations for supporting diagnosis, such as body type, posture and movement, the smell of body fluid, and manifestations of the human spirit.

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14

Gabor, Patonay, and Society of Photo-optical Instrumentation Engineers., eds. Longer wavelength lasers and applications: 27-28 January 1994, Los Angeles, California. Bellingham, Wash., USA: SPIE, 1994.

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15

A, Remillard Ronald, Woo Jonathan W, and United States. National Aeronautics and Space Administration., eds. ROSAT observations of a new X-ray transient in the small Magellanic cloud. [Washington, DC: National Aeronautics and Space Administration, 1997.

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16

Henriksen, Niels Engholm, and Flemming Yssing Hansen. Unimolecular Reactions. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198805014.003.0007.

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This chapter considers unimolecular reactions; photo-induced reactions, that is, true unimolecular reactions; and reactions initiated by collisional activation, that is, apparent unimolecular reactions where it is assumed that the time scales for activation and subsequent reaction are well separated. Elements of classical and quantum dynamical descriptions are discussed, including Slater theory and the quantum mechanical description of photo-induced reactions. Statistical theories aiming at the calculation of micro-canonical as well as canonical rate constants are discussed, including a detailed discussion of RRKM theory. It concludes with a discussion of femtochemistry, that is, the observation and control of chemical dynamics using femtosecond pulses of electromagnetic radiation, focusing on the control of unimolecular reactions via the interaction with coherent light; that is, laser control.

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17

United States. National Aeronautics and Space Administration., ed. Multiwavelength observations of unidentified high energy gamma-ray sources: Annual status report for NAG 5-2051. [Washington, D.C.]: National Aeronautics and Space Administration, 1995.

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18

United States. National Aeronautics and Space Administration., ed. Multiwavelength observations of unidentified high energy gamma-ray sources: Annual status report for NAG 5-2051. [Washington, D.C.]: National Aeronautics and Space Administration, 1995.

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19

United States. National Aeronautics and Space Administration., ed. Multiwavelength observations of unidentified high energy gamma-ray sources: Combined annual status report & final technical report for NAG 5-2051. [Washington, DC: National Aeronautics and Space Administration, 1993.

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20

United States. National Aeronautics and Space Administration., ed. Multiwavelength observations of unidentified high energy gamma-ray sources: Combined annual status report & final technical report for NAG 5-2051. [Washington, DC: National Aeronautics and Space Administration, 1993.

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21

News, World Spaceflight. 21st Century Complete Guide to the Chandra X-Ray Observatory ¿ Images and X-ray Astronomy Scientific Observations of Supernovae, Pulsars, Neutron Stars, Quasars, Galaxies, Clusters, Black Holes, and the Milky Way ¿ Images and Movies. Progressive Management, 2003.

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22

Lefaucheur, Jean-Pascal. TMS and pain. Edited by Charles M. Epstein, Eric M. Wassermann, and Ulf Ziemann. Oxford University Press, 2012. http://dx.doi.org/10.1093/oxfordhb/9780198568926.013.0046.

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Few clinical investigations show that repeated transcranial magnetic stimulation (rTMS) to the brain could produce analgesia. Apart from the relationship between TMS and pain with respect to the clinical observation of rTMS-induced analgesic effects, this article also reviews the effects of pain on motor cortex excitability assessed by single or paired-pulse TMS and the results obtained by applying peripheral magnetic stimulation to treat musculoskeletal pain. This article discusses the effects of acute phasic provoked pain, and prolonged tonic provoked pain on motor cortex excitability. The analgesic effects resulting from a single session of rTMS are too short-lived and thereby incompatible with a durable control of chronic pain. Repeated sessions of rTMS on consecutive days produce cumulative effects. However, repeated daily rTMS sessions can be applied to control pain syndromes for a limited period. Further work is needed to define the ultimate clinical role of TMS in the management of pain.

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23

Romagnoli, Stefano, and Giovanni Zagli. Blood pressure monitoring in the ICU. Oxford University Press, 2016. http://dx.doi.org/10.1093/med/9780199600830.003.0131.

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Two major systems are available for measuring blood pressure (BP)—the indirect cuff method and direct arterial cannulation. In critically-ill patients admitted to the intensive care unit, the invasive blood pressure is the ‘gold standard’ as a tight control of BP values, and its change over time is important for choosing therapies and drugs titration. Since artefacts due to the inappropriate dynamic responses of the fluid-filled monitoring systems may lead to clinically relevant differences between actual and displayed pressure values, before considering the BP value shown as reliable, the critical care giver should carefully evaluate the presence/absence of artefacts (over- or under-damping/resonance). After the arterial pressure waveform quality has been verified, the observation of each component of the arterial wave (systolic upstroke, peak, systolic decline, small pulse of reflected pressure waves, dicrotic notch) may provide a number of useful haemodynamic information. In fact, changes in the arterial pulse contour are due the interaction between the heart beat and the whole vascular properties. Vasoconstriction, vasodilatation, shock states (cardiogenic, hypovolaemic, distributive, obstructive), valve diseases (aortic stenosis, aortic regurgitation), ventricular dysfunction, cardiac tamponade are associated with particular arterial waveform characteristics that may suggest to the physician underlying condition that could be necessary to investigate properly. Finally, the effects of positive-pressure mechanical ventilation on heart–lung interaction, may suggest the existence of an absolute or relative hypovolaemia by means of the so-called dynamic indices of fluid responsiveness.

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24

Raghunathan, Karthik, and Andrew Shaw. Crystalloids in critical illness. Oxford University Press, 2016. http://dx.doi.org/10.1093/med/9780199600830.003.0057.

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‘Crystalloid’ refers to solutions of crystalline substances that can pass through a semipermeable membrane and are distributed widely in body fluid compartments. The conventional Starling model predicts transvascular exchange based on the net balance of opposing hydrostatic and oncotic forces. Based on this model, colloids might be considered superior resuscitative fluids. However, observations of fluid behaviour during critical illness are not consistent with such predictions. Large randomized controlled studies have consistently found that colloids offer no survival advantage relative to crystalloids in critically-ill patients. A revised Starling model describes a central role for the endothelial glycocalyx in determining fluid disposition. This model supports crystalloid utilization in most critical care settings where the endothelial surface layer is disrupted and lower capillary pressures (hypovolaemia) make volume expansion with crystalloids effective, since transvascular filtration decreases, intravascular retention increases and clearance is significantly reduced. There are important negative consequences of both inadequate and excessive crystalloid resuscitation. Precise dosing may be titrated based on functional measures of preload responsiveness like pulse pressure variation or responses to manoeuvres such as passive leg raising. Crystalloids have variable electrolyte concentrations, volumes of distribution, and, consequently variable effects on plasma pH. Choosing balanced crystalloid solutions for resuscitation may be potentially advantageous versus ‘normal’ (isotonic, 0.9%) saline solutions. When used as the primary fluid for resuscitation, saline solutions may have adverse effects in critically-ill patients secondary to a reduction in the strong ion difference and hyperchloraemic, metabolic acidosis. Significant negative effects on immune and renal function may result as well.

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25

America, Optical Society of, ed. Fourier transform spectroscopy: February 10-12, 1997, Hilton Hotel, Santa Fe, New Mexico. Washington, DC: The Society, 1997.

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26

T. Wave Phenomena. Courier Dover Publications, 2014.

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