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Relevant bibliographies by topics / Ashman

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Journal articles

Academic literature on the topic 'Ashman'

Author: Grafiati

Published: 20 April 2024

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Journal articles on the topic "Ashman"

1

Lawler, John. "Reply to Ian Ashman." Leadership 3, no. 1 (2007): 107–13. http://dx.doi.org/10.1177/1742715007073069.

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2

Atzenbeck, Claus. "Interview with Helen Ashman." ACM SIGWEB Newsletter, Summer (July 6, 2016): 1–3. http://dx.doi.org/10.1145/2956573.2956575.

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3

Singla, V., B. Singh, Y. Singh, and C. N. Manjunath. "Ashman phenomenon: a physiological aberration." Case Reports 2013, may24 1 (2013): bcr2013009660. http://dx.doi.org/10.1136/bcr-2013-009660.

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4

Hulick, Jeannette. "Henry Wants More! by Linda Ashman." Bulletin of the Center for Children's Books 69, no. 6 (2016): 294. http://dx.doi.org/10.1353/bcc.2016.0088.

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5

Akiyama, Toshio, J. Franklin Richeson, Robert T. Faillace, Jeffrey Lockhart, and Joel C. Scherer. "Ashman phenomenon of the T wave." American Journal of Cardiology 63, no. 12 (1989): 886–90. http://dx.doi.org/10.1016/0002-9149(89)90069-6.

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6

Brodie, Jean P. "Proto–Globular Cluster Candidates in NGC 1275." Symposium - International Astronomical Union 186 (1999): 273–74. http://dx.doi.org/10.1017/s0074180900112744.

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The discovery, with HST imaging, of proto–globular cluster candidates in NGC 1275 (Holtzman et al. 1992) was regarded by many as a major success of the merger model for globular cluster formation (e.g. Ashman & Zepf 1992) and has been cited in support of the idea that elliptical galaxies form from the merger of two or more spiral galaxies. A prediction of the Ashman & Zepf model was that newly-formed clusters should be observable in currently or recently merging systems. The NGC 1275 clusters constitute an important test of globular cluster formation models. NGC 1275 is the peculiar cD

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7

Goodin, Douglas S., and Anthony T. Reder. "Response to GS Gronseth and E Ashman." Multiple Sclerosis Journal 18, no. 11 (2012): 1661–62. http://dx.doi.org/10.1177/1352458512463484.

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8

Stevenson, Deborah. "When the Storm Comes by Linda Ashman." Bulletin of the Center for Children's Books 73, no. 9 (2020): 388. http://dx.doi.org/10.1353/bcc.2020.0336.

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9

Chaudry, Imran I., Eddison K. Ramsaran, and David H. Spodick. "Observations on the reliability of the Ashman phenomenon." American Heart Journal 128, no. 1 (1994): 205–9. http://dx.doi.org/10.1016/0002-8703(94)90034-5.

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10

Zepf, Stephen E., and Keith M. Ashman. "Globular Cluster Systems of Elliptical Galaxies." Symposium - International Astronomical Union 186 (1999): 173–80. http://dx.doi.org/10.1017/s0074180900112483.

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We review the observed properties of globular cluster systems and their implications for models of galaxy formation. Observations show that globular clusters form in gas-rich mergers, and that bimodal metallicity distributions are common in the globular cluster systems of ellipticals, with the metal-poor population more extended than the metal-rich one. These are three of the four predictions of the simple merger model of Ashman & Zepf (1992). The fourth prediction concerns the properties of the globular cluster systems of spirals, and is still to be tested by observation. Adopting Occam's

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