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    101. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_22_97
    ... Deep Imaging of Globular Clusters in the Coma Ellipticals) The WF/PC-2 was used to make deep observations of the central nuclear region in super giant elliptical galaxy NGC-4874 which is located in the Coma Galactic Cluster looking for globular clusters ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_22_97 -- 8.8 Кб -- 22.07.1997
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    102. The Hubble Constant via the Leo-I Group
    ... The two routes from Leo-I to Coma rely mainly on various early-type galaxy distance ... The Coma cluster is assumed to be sufficiently remote that the corrections to its ... Stepping from Leo-I to Coma, TSFR infer a value for of (see figure 1). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/tanvirn.html -- 19.7 Кб -- 15.06.2005
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    103. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_06_24_96
    ... 1.6 Completed WF/PC-2 5997 (The Cores of Elliptical Galaxies in the = Coma Cluster) The WF/PC-2 was used to make observations of the large elliptical = galaxies GAL-125054 and IC832 which are located in the Coma Cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_06_24_96 -- 11.9 Кб -- 24.06.1996
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    104. http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr9505.pdf
    ... a single chip due to obscuration shifting, focus, coma, and astigmatism changes ... o set caused by the bounce results in coma induced by the corrective optics in WFPC2 ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr9505.pdf -- 527.3 Кб -- 05.02.2013
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    105. http://www.stsci.edu/hst/wfpc2/documents/tir/TIR/tir_9703.pdf
    ... mirror displacement (positive if the secondary was too far away from the primary), 8) the focus position, after correction for OTA breathing, 9) and 10) the x and y component of the image coma, in micron rms at the focal plane, and 11) the filter used ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfpc2/documents/tir/TIR/tir_9703.pdf -- 285.0 Кб -- 03.12.2008
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    106. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_23_95
    ... The WF/PC-2 was used to attempt to make deep images of the elliptical galaxy 0023+171 which is a member of the Coma Cluster ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_23_95 -- 9.5 Кб -- 23.01.1995
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    107. HST this week: 352
    ... Origin of UCDs in the Coma Cluster . 12926 . ... GO 12918: Origin of UCDs in the Coma Cluster . ... The Coma cluster is the nearest rich galaxy cluster, lying at a distance of ~100 Mpc ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2012/thisweek352.html -- 20.0 Кб -- 24.11.2014
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    108. http://www.stsci.edu/hst/observatory/documents/Makidon_et_al_SPIE2006
    ... Because order coma, astigmatism instruments at that instr of it's Ritchey-Chretian design, HST trades third-order coma and ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/observatory/documents/Makidon_et_al_SPIE2006 -- 573.4 Кб -- 13.10.2006
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    109. HST this week: 023
    ... The aim of the present project is to extend covrage to Cepheids within the Coma cluster. ... If Coma lies at a distance of 100 Mpc ( (m-M)=35.0), then long-period Cepheids (P~50 days) have mean apparent magnitudes of V ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2012/thisweek023.html -- 16.0 Кб -- 30.01.2012
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    110. JWST SODRM Solar System Programs Summary
    ... The SNR for these objects was estimated by computing the surface brightness expected from the coma (assuming an optical depth of 10 -4 ), converting that into an equivalent point-source flux, and adding the coma and nucleus contributions. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/jwst/science/sodrm/Solar-System-Science-Programs-summary -- 64.6 Кб -- 11.04.2016
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