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Journal articles on the topic 'Virgo'

Author: Grafiati

Published: 4 June 2021

Last updated: 26 July 2025

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1

Olchanski, M., and J. G. Sorce. "Merger types forming the Virgo cluster in recent gigayears." Astronomy & Astrophysics 614 (June 2018): A102. http://dx.doi.org/10.1051/0004-6361/201731911.

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Context. As our closest cluster-neighbor, the Virgo cluster of galaxies is intensely studied by observers to unravel the mysteries of galaxy evolution within clusters. At this stage, cosmological numerical simulations of the cluster are useful to efficiently test theories and calibrate models. However, it is not trivial to select the perfect simulacrum of the Virgo cluster to fairly compare in detail its observed and simulated galaxy populations that are affected by the type and history of the cluster. Aims. Determining precisely the properties of Virgo for a later selection of simulated clust

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2

East, Charles. "Virgo." Sewanee Review 121, no. 1 (2013): 18–26. http://dx.doi.org/10.1353/sew.2013.0002.

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3

Zaragoza, Gabrijela Mecky. "Virgo und Virago: Zwei Frühneuzeitliche Judith-Figuren im Vergleich." Daphnis 31, no. 1-2 (2002): 107–26. http://dx.doi.org/10.1163/18796583-0310102005.

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Die These des Artikels ist, daß der konfessionell geprägte Paradigmenwechsel im frühneuzeitlichen weiblichen Gendermodell Auswirkungen darauf hat, wie die ersten beiden Judith-Texte des 16. Jahrhunderts – Marko Marulićs Judita (1501) und Sixt Bircks lvdith (1534) – mit ihren mörderischen Heldinnen umgehen. Während Marulićs Text selbstbewußt das Bild einer Renaissancemadonna feiert, macht sich in Bircks Text Verwirrung breit. Der Widerspruch zwischen dem verhäuslichten weiblichen Frauenbild der Zwingli-Ära und dem eigentlichen - von Martin Luther als “fein/ gut/ nuetzlich” klassifizierten – Jud

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4

Li, Gege. "Virgo 3.0." New Scientist 249, no. 3317 (2021): 29. http://dx.doi.org/10.1016/s0262-4079(21)00061-0.

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5

Castignani, G., F. Combes, P. Jablonka, et al. "Virgo filaments." Astronomy & Astrophysics 657 (December 21, 2021): A9. http://dx.doi.org/10.1051/0004-6361/202040141.

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It is now well established that galaxies have different morphologies, gas contents, and star formation rates (SFR) in dense environments like galaxy clusters. The impact of environmental density extends to several virial radii, and galaxies appear to be pre-processed in filaments and groups before falling into the cluster. Our goal is to quantify this pre-processing in terms of gas content and SFR, as a function of density in cosmic filaments. We have observed the two first CO transitions in 163 galaxies with the IRAM-30 m telescope, and added 82 more measurements from the literature, thus for

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6

Undheim, Sissel. "Christus Virgo." Bulletin for the Study of Religion 41, no. 2 (2012): 22–27. http://dx.doi.org/10.1558/bsor.v41i2.22.

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The description of Christ as a virgin, 'Christus virgo', does occur at rare occasions in Early Christian and late antique texts. Considering that 'virgo' was a term that most commonly described the sexual and moral status of a member of the female sex, such representations of Christ as a virgin may exemplify some of the complex negotiations over gender, salvation, sanctity and Christology that we find in the writings of the Church fathers. The article provides some suggestions as to how we can understand the notion of the virgin Christ within the context of early Christian and late antique the

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7

Acernese, F., M. Alshourbagy, P. Amico, et al. "Virgo status." Classical and Quantum Gravity 25, no. 18 (2008): 184001. http://dx.doi.org/10.1088/0264-9381/25/18/184001.

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8

Haines, John. "New light on the polyphonic sequence Ave virgo, virga Jesse." Early Music 34, no. 1 (2006): 55–74. http://dx.doi.org/10.1093/em/cah191.

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9

Tanaka, Kazuhisa I. "The Structure of the Virgo Cluster of Galaxies." Publications of the Astronomical Society of Japan 37, no. 1 (1985): 133–54. https://doi.org/10.1093/pasj/37.1.133.

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Abstract A new detailed analysis of galaxies in the Virgo area shows that the conventional Virgo cluster comprises two different clouds of galaxies: the Virgo cluster I and the Southern cloud II by our definition. Excluding the galaxies in the Southern cloud II, the Virgo cluster I centered at 12h27m.16, + 13°07′ (1950), has a mean radial velocity of ⟨V0⟩ ≃+ 980 ± 60 km s–1 and there is no significant velocity difference between elliptical-lenticular and spiral-irregular galaxies in the Virgo cluster I. The Southern cloud II is centered at about 12h25m, + 7°30′ (1950) and all types of galaxies

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10

Chung, Jiwon, Suk Kim, Soo-Chang Rey, and Youngdae Lee. "Star-forming Dwarf Galaxies in Filamentary Structures around the Virgo Cluster: Probing Chemical Pre-processing in Filament Environments." Astrophysical Journal 923, no. 2 (2021): 235. http://dx.doi.org/10.3847/1538-4357/ac3002.

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Abstract It has been proposed that the filament environment is closely connected to the pre-processing of galaxies, where their properties may have been changed by environmental effects in the filament before they fell into the galaxy cluster. We present the chemical properties of star-forming dwarf galaxies (SFDGs) in five filamentary structures (Virgo III, Leo Minor, Leo II A, Leo II B, and Canes Venatici) around the Virgo cluster using the Sloan Digital Sky Survey optical spectroscopic data and Galaxy Evolution Explorer ultraviolet photometric data. We investigate the relationship between s

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11

Ummul Aini, Dzul Afria Sari, and Fadhila Yusri. "PERAN KELURGA DALAM MENDUKUNG READINESS SISWA (Studi Kasus Pada Siswa Sekolah Dasar Islam Excellent)." Jurnal Pendidikan dan Kebudayaan (JURDIKBUD) 3, no. 2 (2023): 322–26. http://dx.doi.org/10.55606/jurdikbud.v3i2.1933.

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Keberhasilan siswa dalam pembelajaran ditentukan oleh banyak faktor, salah satunya kesiapan dalam belajar. Kesiapan siswa dalam belajar dapat dilihat dari, kesiapan fisik, kesiapan mental, motivasi, pengetahuan atau materi pembelajaran, bahan ajar dan juga alat alat yang mendukung pembelajaran. Tujuan penelitian untuk mengetahui penyebab dan solusi dari permasalahan yang dihadapi oleh Virgo. Jenis penelitianya Case Study atau Studi Kasus, dimana studi kasus ini adalah salah satu bentuk penelitian kualitatif yang berbasis pada pemahaman dan perilaku manusia berdasarkan opini manusia. Sabjek dal

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12

Raffi, François, Véronique Reliquet, Virginie Ferré, et al. "The Virgo Study: Nevirapine, Didanosine and Stavudine Combination Therapy in Antiretroviral-Naive HIV-1-Infected Adults." Antiviral Therapy 5, no. 4 (1999): 267–72. http://dx.doi.org/10.1177/135965350000500405.

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The virological and immunological efficacy of the triple regimen containing nevirapine (once or twice daily), didanosine (once daily) and stavudine, in antiretroviral-naive patients infected with HIV-1, was evaluated in an open-label, prospective, non-randomized, multi-centre, 52-week study. The first 60 patients (VIRGO I) received nevirapine as the standard dose, 200 mg twice daily; the subsequent 40 patients (VIRGO II) received nevirapine at a dose of 400 mg once daily. All patients received 400 mg of didanosine once daily and 40 mg of stavudine twice daily, adjusted for body weight. At base

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13

Hellemans, Alexander. "View from VIRGO." Scientific American 289, no. 2 (2003): 25–26. http://dx.doi.org/10.1038/scientificamerican0803-25.

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14

ALCOCQ, A. "Aquarius and Virgo." Le Muséon 99, no. 3 (1986): 249–50. http://dx.doi.org/10.2143/mus.99.3.2011467.

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15

Acernese, F., P. Amico, M. Alshourbagy, et al. "Virgo upgrade investigations." Journal of Physics: Conference Series 32 (March 2, 2006): 223–29. http://dx.doi.org/10.1088/1742-6596/32/1/033.

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16

Acernese, F., P. Amico, M. Al-Shourbagy, et al. "Status of Virgo." Classical and Quantum Gravity 22, no. 18 (2005): S869—S880. http://dx.doi.org/10.1088/0264-9381/22/18/s01.

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17

Acernese, F., P. Amico, M. Alshourbagy, et al. "The Virgo status." Classical and Quantum Gravity 23, no. 19 (2006): S635—S642. http://dx.doi.org/10.1088/0264-9381/23/19/s01.

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18

Acernese, F., M. Alshourbagy, P. Amico, et al. "Status of Virgo." Classical and Quantum Gravity 25, no. 11 (2008): 114045. http://dx.doi.org/10.1088/0264-9381/25/11/114045.

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19

Braccini), The VIRGO Collaboration (presented. "The VIRGO suspensions." Classical and Quantum Gravity 19, no. 7 (2002): 1623–29. http://dx.doi.org/10.1088/0264-9381/19/7/353.

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20

Collaboration:, The VIRGO, F. Acernese, P. Amico, et al. "Status of VIRGO." Classical and Quantum Gravity 20, no. 17 (2003): S609—S616. http://dx.doi.org/10.1088/0264-9381/20/17/304.

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21

Acernese, F., P. Amico, N. Arnaud, et al. "Status of VIRGO." Classical and Quantum Gravity 21, no. 5 (2004): S385—S394. http://dx.doi.org/10.1088/0264-9381/21/5/002.

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22

Acernese, F., P. Amico, M. Alshourbagy, et al. "Status of Virgo." Journal of Physics: Conference Series 39 (May 1, 2006): 32–35. http://dx.doi.org/10.1088/1742-6596/39/1/007.

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23

Acernese, F., T. Adams, K. Agatsuma, et al. "Advanced Virgo Status." Journal of Physics: Conference Series 1342 (January 2020): 012010. http://dx.doi.org/10.1088/1742-6596/1342/1/012010.

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24

Gomes da Rocha, Francisco. "Virgo Prudentissima (Antífona)." Revista Música 4, no. 2 (1993): 139. http://dx.doi.org/10.11606/rm.v4i2.55065.

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25

Mould, Jeremy. "The Virgo Cluster." Proceedings of the International Astronomical Union 8, S289 (2012): 262–68. http://dx.doi.org/10.1017/s1743921312021527.

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AbstractIn the era of precision cosmology, the Virgo cluster takes on a new role in the cosmic distance scale. Its traditional role of testing the consistency of secondary distance indicators is replaced by an ensemble of distance measurements within the Local Supercluster, united by a velocity-field model obtained from a reconstruction based on redshift surveys. The Wilkinson Microwave Anisotropy Probe (WMAP) leads us to see the Hubble constant as one of six parameters in a standard model of cosmology with considerable covariance among parameters. Independent experiments, such as WMAP, the Hu

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26

Guite, Malcolm. "O Virgo Virginum." Spiritus: A Journal of Christian Spirituality 18, no. 2 (2018): 269. http://dx.doi.org/10.1353/scs.2018.0036.

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27

Bersanetti, Diego, Barbara Patricelli, Ornella Juliana Piccinni, Francesco Piergiovanni, Francesco Salemi, and Valeria Sequino. "Advanced Virgo: Status of the Detector, Latest Results and Future Prospects." Universe 7, no. 9 (2021): 322. http://dx.doi.org/10.3390/universe7090322.

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The Virgo detector, based at the EGO (European Gravitational Observatory) and located in Cascina (Pisa), played a significant role in the development of the gravitational-wave astronomy. From its first scientific run in 2007, the Virgo detector has constantly been upgraded over the years; since 2017, with the Advanced Virgo project, the detector reached a high sensitivity that allowed the detection of several classes of sources and to investigate new physics. This work reports the main hardware upgrades of the detector and the main astrophysical results from the latest five years; future prosp

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28

Pierce, M. J., R. D. McClure, D. L. Welch, R. Racine, and S. van den Bergh. "Cepheid and Long – Period Variables in Virgo Cluster Galaxies." International Astronomical Union Colloquium 139 (1993): 81–89. http://dx.doi.org/10.1017/s0252921100116938.

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AbstractWe are currently undertaking a ground-based imaging survey which attempts to discover and determine periods for variable stars in Virgo Cluster galaxies. Such a survey is now feasible thanks to the high resolution imaging (FWHM ≤ 0.50 arcsec) routinely obtained with the High Resolution Camera on the Canada-France-Hawaii Telescope. The Virgo Cluster has long been considered a crucial “stepping-stone” in the extragalactic distance scale problem given that the cluster is at a “cosmologically interesting” distance and that there is little controversy in the relative distance between Virgo

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29

Anand, Gagandeep S., R. Brent Tully, Yotam Cohen, et al. "The TRGB–SBF Project. II. Resolving the Virgo Cluster with JWST." Astrophysical Journal 982, no. 1 (2025): 26. https://doi.org/10.3847/1538-4357/adb399.

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Abstract The Virgo Cluster is the nearest substantial cluster of galaxies to the Milky Way and a cornerstone of the extragalactic distance scale. Here, we present JWST/NIRCam observations that simultaneously cover the cores and halos of 10 galaxies in and around the Virgo Cluster and are designed to perform simultaneous measurements of the tip of the red giant branch (TRGB) and surface brightness fluctuations (SBF). Seven of the targets are within the Virgo Cluster and where we are able to resolve some of the cluster’s substructure, while an additional three provide important constraints on Vi

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30

Mihos, J. Christopher, Patrick R. Durrell, Elisa Toloba, et al. "The Distance and Dynamical History of the Virgo Cluster Ultradiffuse Galaxy VCC 615." Astrophysical Journal 924, no. 2 (2022): 87. http://dx.doi.org/10.3847/1538-4357/ac35d9.

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Abstract We use deep Hubble Space Telescope imaging to derive a distance to the Virgo Cluster ultradiffuse galaxy (UDG) VCC 615 using the tip of the red giant branch (TRGB) distance estimator. We detect 5023 stars within the galaxy, down to a 50% completeness limit of F814W ≈ 28.0, using counts in the surrounding field to correct for contamination due to background sources and Virgo intracluster stars. We derive an extinction-corrected F814W tip magnitude of m tip , 0 = 27.19 − 0.05 + 0.07 , yielding a distance of d = 17.7 − 0.4 + 0.6 Mpc. This places VCC 615 on the far side of the Virgo Clust

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31

Moreno, Lara. "EL VIRGO Y EL LEÓN." Revista Internacional de Culturas y Literaturas 6, no. 6 (2007): 44–47. http://dx.doi.org/10.12795/ricl.2007.i06.06.

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32

Acernese, F., T. Adams, K. Agatsuma, et al. "Status of the Advanced Virgo gravitational wave detector." International Journal of Modern Physics A 32, no. 28n29 (2017): 1744003. http://dx.doi.org/10.1142/s0217751x17440031.

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Advanced Virgo is the French–Italian second generation laser gravitational wave detector, successor of the Initial Virgo. This new interferometer keeps only the infrastructure of its predecessor and aims to be ten times more sensitive, with its first science run planned for 2017. This article gives an overview of the Advanced Virgo design and the technical choices behind it. Finally, the up-to-date progresses and the planned upgrade for the following years are detailed.

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33

Talabishka, Evgeniy, Alexander Didenko, and Igor Velykopolskiy. "Some biological data on cactus roach, Rutilus virgo (Heckel), in rivers of the Transcarpathian region of Ukraine." Archives of Polish Fisheries 23, no. 2 (2015): 67–77. http://dx.doi.org/10.1515/aopf-2015-0008.

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Abstract The occurrence of Rutilus virgo (Heckel) has been confirmed in the Transcarpathian region of Ukraine, where it was caught in the lower stretches of the Latorica and Borzhava rivers. The comparison of selected morphometric features of R. rutilus and R. virgo showed that 26 of 40 of them were significantly different and the largest differences were observed for features such as head length, maximum body depth, pectoral fin length, pectoral fin thickness, pelvic fin length, head depth at eye level, maximum head depth, and preorbital length. The comparison of R. virgo of two size groups s

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34

Côté, Patrick, and Michael J. West. "The ACS Virgo Cluster Survey." Highlights of Astronomy 13 (2005): 179–80. http://dx.doi.org/10.1017/s1539299600015537.

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AbstractWe describe the ACS Virgo Cluster Survey, an HST imaging survey of early-type galaxies in the Virgo Cluster. Multi-color ACS images for one hundred member galaxies, spanning a range of 450 in luminosity, are being used to study the central regions of these galaxies, their globular cluster systems, and the three-dimensional structure of Virgo itself. In terms of depth, spatial resolution, sample size and homogeneity, this represents the most comprehensive imaging survey to date of early-type galaxies in dense environments.

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35

Kashibadze, Olga G., Igor D. Karachentsev, and Valentina E. Karachentseva. "Structure and kinematics of the Virgo cluster of galaxies." Astronomy & Astrophysics 635 (March 2020): A135. http://dx.doi.org/10.1051/0004-6361/201936172.

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Aims. This work considers the Virgo cluster of galaxies, focusing on its structure, kinematics, and morphological landscape. Our principal aim is to estimate the virial mass of the cluster. For this purpose, we present a sample of 1537 galaxies with radial velocities VLG < 2600 km s−1 situated within a region of ΔSGL = 30° and ΔSGB = 20° around M 87. About half of the galaxies have distance estimates. Methods. We selected 398 galaxies with distances in a (17 ± 5) Mpc range. Based on their 1D and 2D number-density profiles and their radial velocity dispersions, we made an estimate for the vi

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36

Nardecchia, Ilaria. "Detecting Gravitational Waves with Advanced Virgo." Galaxies 10, no. 1 (2022): 28. http://dx.doi.org/10.3390/galaxies10010028.

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Advanced Virgo is the European gravitational-wave detector that, along with the American ones, is part of the global network of detectors that have been pinpointing gravitational waves since 2015. These kilometer-scale laser interferometers, measuring the distance between quasi-free-falling mirrors, represent the suitable detectors to explore the Universe through gravitational radiation. The initial Virgo experiment completed several runs of scientific data between 2007 and 2011, establishing the upper limits on the gravitational-wave rate expected for several astrophysical sources. The Advanc

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37

Mantovani, Maddalena. "Virgo and the gravitational interferometry." EPJ Web of Conferences 280 (2023): 08005. http://dx.doi.org/10.1051/epjconf/202328008005.

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The Advanced Virgo detector is a long scale enhanced Michelson interferometer placed in Italy, close to Pisa, with the aim of detecting gravitational waves from astronomical sources. The Advanced Virgo interferometer has detected, together with the LIGO interferometers located in USA [1], an impressive collection of gravitational waves emissions in the last observation runs O2 and O3. During the last observation run (O3), which lasted about one year of data taking from April 2019 to March 2020, were detected about 80 events. When the run ended, the detector has been upgraded toward the Advance

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38

Donlon, Thomas, Heidi Jo Newberg, Jake Weiss, Paul Amy, and Jeffery Thompson. "The Virgo Overdensity Explained." Astrophysical Journal 886, no. 2 (2019): 76. http://dx.doi.org/10.3847/1538-4357/ab4f72.

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39

Isi, Maximiliano. "Recent LIGO-Virgo discoveries." Modern Physics Letters A 36, no. 11 (2021): 2130010. http://dx.doi.org/10.1142/s021773232130010x.

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The LIGO and Virgo gravitational-wave detectors carried out the first half of their third observing run from April through October 2019. During this period, they detected 39 new signals from the coalescence of black holes or neutron stars, more than quadrupling the total number of detected events. These detections included some unprecedented sources, like a pair of black holes with unequal masses (GW190412), a massive pair of neutron stars (GW190425), a black hole potentially in the supernova pair-instability mass gap (GW190521), and either the lightest black hole or the heaviest neutron star

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40

Beall, Abigail. "Hunting Leo and Virgo." New Scientist 250, no. 3334 (2021): 51. http://dx.doi.org/10.1016/s0262-4079(21)00844-7.

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41

PALCA, J. "A Surprise Near Virgo." Science 245, no. 4921 (1989): 933. http://dx.doi.org/10.1126/science.245.4921.933.

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42

van der Schaaf, L., K. Agatsuma, M. van Beuzekom, M. Gebyehu, and J. van den Brand. "Advanced Virgo phase cameras." Journal of Physics: Conference Series 718 (May 2016): 072008. http://dx.doi.org/10.1088/1742-6596/718/7/072008.

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43

Acernese, F., P. Amico, M. Al-Shourbagy, et al. "The status of VIRGO." Classical and Quantum Gravity 23, no. 8 (2006): S63—S69. http://dx.doi.org/10.1088/0264-9381/23/8/s09.

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44

Acernese, F., P. Amico, M. Alshourbagy, et al. "Status of Virgo detector." Classical and Quantum Gravity 24, no. 19 (2007): S381—S388. http://dx.doi.org/10.1088/0264-9381/24/19/s01.

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45

Acernese, F., T. Adams, K. Agatsuma, et al. "Status of Advanced Virgo." EPJ Web of Conferences 182 (2018): 02003. http://dx.doi.org/10.1051/epjconf/201818202003.

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The LIGO and the Virgo collaborations have recently announced the first detections of Gravitational Waves. Due to their weak amplitude, Gravitational Waves are expected to produce a very small effect on free-falling masses, which undergo a displacement of the order of 10-18 m for a Km-scale mutual distance. This discovery showed that interferometric detectors are suitable to reveal such a feeble effect, and therefore represent a new tool for astronomy, astrophysics and cosmology in the understanding of the Universe. To better reconstruct the position of the Gravitational Wave source and increa

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46

Bondu, F., A. Brillet, F. Cleva, et al. "The VIRGO injection system." Classical and Quantum Gravity 19, no. 7 (2002): 1829–33. http://dx.doi.org/10.1088/0264-9381/19/7/381.

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47

Tournefier, E., and the VIRGO Collaboration. "The status of virgo." Journal of Physics: Conference Series 110, no. 6 (2008): 062025. http://dx.doi.org/10.1088/1742-6596/110/6/062025.

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48

Acernese, F., T. Adams, M. Agathos, et al. "The Advanced Virgo detector." Journal of Physics: Conference Series 610 (May 11, 2015): 012014. http://dx.doi.org/10.1088/1742-6596/610/1/012014.

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49

Hochreiter, Eduard H. "John Virgo: Fond Remembrances." International Advances in Economic Research 19, no. 4 (2013): 459–60. http://dx.doi.org/10.1007/s11294-013-9426-z.

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50

Daniels, Joseph. "Memories of John Virgo." International Advances in Economic Research 19, no. 4 (2013): 461–62. http://dx.doi.org/10.1007/s11294-013-9432-1.

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