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Journal articles on the topic 'Chamaeleon'

Author: Grafiati

Published: 10 December 2022

Last updated: 31 July 2025

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1

SEABRA, SOFIA G., INÊS SATAR, and OCTÁVIO S. PAULO. "Microsatellite loci isolated from Chamaeleo chamaeleon." Journal of Genetics 94, S1 (2015): 144–47. http://dx.doi.org/10.1007/s12041-014-0463-z.

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2

Fouda, Yosra A., Dalia A. Sabry, and Dalia F. Abou-Zaid. "Functional Anatomical, Histological and Ultrastructural Studies of three Chameleon Species: Chamaeleo Chamaeleon, Chamaeleo Africanus, and Chamaeleon Vulgaris." International Journal of Morphology 33, no. 3 (2015): 1045–53. http://dx.doi.org/10.4067/s0717-95022015000300038.

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3

Dimaki, Maria, Anna Hundsdörfer, and Uwe Fritz. "Eastern Mediterranean chameleons (Chamaeleo chamaeleon, Ch. africanus) are distinct." Amphibia-Reptilia 29, no. 4 (2008): 535–40. http://dx.doi.org/10.1163/156853808786230415.

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AbstractBased on mitochondrial 16S rRNA sequences, we suggest that the founder individuals of the introduced Greek population of Chamaeleo africanus originated in the Nile Delta region of Egypt. In Ch. chamaeleon, we discovered in the eastern Mediterranean new 16S rRNA haplotypes, being highly distinct from previously published western Mediterranean haplotypes. Eastern Mediterranean haplotypes were found in samples from northern Syria, Cyprus, Crete, Samos, Malta and Tunisia. The occurrence of an eastern Mediterranean haplotype in Tunisia and of distinct haplotypes in Morocco could argue for a

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4

Eshar, David, Roi Lapid, and Valerie Head. "Transilluminated Jugular Blood Sampling in the Common Chameleon (Chamaeleo chamaeleon)." Journal of Herpetological Medicine and Surgery 28, no. 1 (2018): 19. http://dx.doi.org/10.5818/17-10-127.1.

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5

CUADRADO, MARIANO, JOSÉ MARTÍN, and PILAR LÓPEZ. "Camouflage and escape decisions in the common chameleon Chamaeleo chamaeleon." Biological Journal of the Linnean Society 72, no. 4 (2001): 547–54. http://dx.doi.org/10.1111/j.1095-8312.2001.tb01337.x.

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6

Sidhom, Marwa, Khaled Said, Noureddine Chatti, et al. "Karyological and bioinformatic data on the common chameleon Chamaeleo chamaeleon." Data in Brief 30 (June 2020): 105640. http://dx.doi.org/10.1016/j.dib.2020.105640.

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7

Burks, Roger A., Jason L. Mottern, Nicole G. Pownall, Rebeccah Waterworth, and Timothy D. Paine. "First record of Closterocerus chamaeleon, parasitoid of the Eucalyptus Gall Wasp Ophelimus maskelli (Hymenoptera, Chalcidoidea, Eulophidae), in the New World." ZooKeys 504 (May 19, 2015): 149–52. https://doi.org/10.3897/zookeys.504.9728.

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The uniparental parasitoid Closterocerus chamaeleon (Girault) is discovered to be fortuitously present on a population of the invasive Eucalyptus Gall Wasp Ophelimus maskelli (Ashmead) in Riverside, California. This is the first report from the New World of C. chamaeleon, which has proven to be a highly effective natural enemy of O. maskelli in the Mediterranean Basin. The taxonomy and identification of C. chamaeleon is discussed.

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8

Basso, Roberto, Maria Luisa Vannuccini, Luca Nerva, Giuseppe Mazza, Matteo Seno, and Emiliano Mori. "Multiple origins of the common chameleon in southern Italy." Herpetozoa 32, no. () (2019): 11–19. https://doi.org/10.3897/herpetozoa.32.e35611.

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The common chameleon Chamaeleo chamaeleon is a Mediterranean lizard which has been introduced in many islands and its native origin in European countries is debated. Chameleons have been introduced in southern Italy, possibly from the Middle East and Tunisia. We conducted genetic analyses on mitochondrial DNA 16S gene on a larger sample. We observed a multiple origin for the Salento (Apulia, southern Italy) population, with individuals phylogenetically related to populations of North Africa and two areas in the Middle East. Some individuals may have been released before the 1950s and some othe

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9

Baran, İbrahim, Max Kasparek, and Mehmet Öz. "On the occurrence and status of the Chameleon,Chamaeleo chamaeleon, in Turkey." Zoology in the Middle East 2, no. 1 (1988): 52–56. http://dx.doi.org/10.1080/09397140.1988.10637558.

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10

Cuadrado, Mariano. "Mate guarding and social mating system in male common chameleons (Chamaeleo chamaeleon)." Journal of Zoology 255, no. 4 (2006): 425–35. http://dx.doi.org/10.1017/s0952836901001510.

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11

Díaz-Paniagua, Carmen. "Effect of cold temperature on the length of incubation of Chamaeleo chamaeleon." Amphibia-Reptilia 28, no. 3 (2007): 387–92. http://dx.doi.org/10.1163/156853807781374782.

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AbstractCommon chameleon eggs spend the first months of incubation at low temperatures. I incubated eggs of different clutches at 25°C in four treatments with respectively 0, 84, 119 and 149 days of initial cold period (at 14°C). Treatments with longer cold periods had longer total incubation but shorter periods of incubation at 25°C. Eggs which did not experience initial cold period showed low synchronization at hatching. Hatchling body mass and length were influenced by the length of the cold period. Hatchlings were largest and heaviest for cold periods of intermediate length which had simil

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12

Hartigan, Patrick. "New T Tauri stars in Chamaeleon I and Chamaeleon II." Astronomical Journal 105 (April 1993): 1511. http://dx.doi.org/10.1086/116530.

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13

Voirin, Jordan, Carlo F. Manara, and Timo Prusti. "A revised estimate of the distance to the clouds in the Chamaeleon complex using the Tycho–Gaia Astrometric Solution." Astronomy & Astrophysics 610 (February 2018): A64. http://dx.doi.org/10.1051/0004-6361/201731153.

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Context. The determination of the distance to dark star-forming clouds is a key parameter to derive the properties of the cloud itself and of its stellar content. This parameter is still loosely constrained even in nearby star-forming regions. Aim. We want to determine the distances to the clouds in the Chamaeleon-Musca complex and explore the connection between these clouds and the large-scale cloud structures in the Galaxy. Methods. We used the newly estimated distances obtained from the parallaxes measured by the Gaia satellite and included in the Tycho–Gaia Astrometric Solution catalog. Wh

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14

MIRALDO, ANDREIA, ISABEL PINTO, JOÃO PINHEIRO, INÊS ROSÁRIO, MARTA MAYMONE, and OCTÁVIO S. PAULO. "NOTE: DISTRIBUTION AND CONSERVATION OF THE COMMON CHAMAELEO CHAMAELEON, IN ALGARVE, SOUTHERN PORTUGAL." Israel Journal of Zoology 51, no. 2 (2005): 157–64. http://dx.doi.org/10.1560/ev2y-9e2f-5dly-p00n.

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15

Cuadrado, Mariano, and Jon Loman. "The Effects of Age and Size on Reproductive Timing in Female Chamaeleo chamaeleon." Journal of Herpetology 33, no. 1 (1999): 6. http://dx.doi.org/10.2307/1565536.

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16

Andrews, Robin M., Carmen Díaz‐Paniagua, Adolfo Marco, and Alexandre Portheault. "Developmental Arrest during Embryonic Development of the Common Chameleon (Chamaeleo chamaeleon) in Spain." Physiological and Biochemical Zoology 81, no. 3 (2008): 336–44. http://dx.doi.org/10.1086/529449.

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17

Keren-Rotem, Tammy, Amos Bouskila, and Eli Geffen. "Ontogenetic habitat shift and risk of cannibalism in the common chameleon (Chamaeleo chamaeleon)." Behavioral Ecology and Sociobiology 59, no. 6 (2005): 723–31. http://dx.doi.org/10.1007/s00265-005-0102-z.

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18

Mouhsine, Touria, Fethi Amani, and Abdeslam Mikdad. "Agama bibronii (Sauria : Agamidae) et Chamaeleo chamaeleon (Sauria : Chamaeleonidae) d’Ifri n’Ammar (Rif oriental, Maroc)." Quaternaire, no. 33/3 (September 1, 2022): 151–68. http://dx.doi.org/10.4000/quaternaire.16948.

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19

Franco, G. A. P. "The Chamaeleon Dark Clouds Complex: Preliminary Analysis of the Colour Excesses E(b-y) Towards the Selected Area 203." International Astronomical Union Colloquium 120 (1989): 133. http://dx.doi.org/10.1017/s0252921100023642.

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The Chamaeleon dark clouds form a large complex of interstellar obscuring material situated at ≈ 15° below the galactic plane. Although it is accepted as being one of the closest low-mass star formation region to the Sun, its distance has been debated issues. The proposed distance is in general dependent on the value assumed for the ratio of total-to-selective extinction, which in the Chamaeleon clouds has proved controversial, leading to distances estimates ranging from 115 to 215 pc.

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20

Liszt, H., M. Gerin, and I. Grenier. "Standing in the shadow of dark gas: ALMA observations of absorption from dark CO in the molecular dark neutral medium of Chamaeleon." Astronomy & Astrophysics 627 (July 2019): A95. http://dx.doi.org/10.1051/0004-6361/201935436.

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Context. We previously detected 89.2 GHz J = 1−0 HCO+ absorption in 12 directions lacking detected CO emission in the outskirts of the Chamaeleon cloud complex and toward one sightline with integrated CO emission WCO = 2.4 K km s−1. Eight sightlines had a much larger mean column density of dark neutral medium (DNM) – gas not represented in HI or CO emission – and were found to have much higher mean molecular column density. The five other sightlines had little or no DNM and were found to have much smaller but still detectable N(HCO+). Aims. To determine the CO column density along previously o

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21

Henning, Th, and E. Thamm. "Cold dust around chamaeleon stars." Astrophysics and Space Science 212, no. 1-2 (1994): 215–20. http://dx.doi.org/10.1007/bf00984525.

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22

Bennis, M., C. Versaux-Botteri, J. Repérant, and J. A. Armengol. "Calbindin, Calretinin and Parvalbumin Immunoreactivity in the Retina of the Chameleon (Chamaeleo chamaeleon)." Brain, Behavior and Evolution 65, no. 3 (2005): 177–87. http://dx.doi.org/10.1159/000083683.

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23

Hassan Nabih Mhanna, Nahla Ibrahim, Aroub Al-Masri, Hassan Nabih Mhanna, Nahla Ibrahim, Aroub Al-Masri. "Modification of preparing the blood diluting solution method and studying the blood cell counts of some Syrian Reptiles and Amphibians using the modified method: تعديل طريقة تحضير المحلول المخفف للدم ودراسة تعداد الخلايا الدموية عند بعض أنواع الزواحف والبرمائيات السورية بالطريقة المعدلة". Journal of natural sciences, life and applied sciences 6, № 1 (2022): 25–35. http://dx.doi.org/10.26389/ajsrp.c071221.

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The study aimed to test the validity of the results of the modified blood diluted solution by Natt-Herrick method in order to study the complete blood count of different blood cells in two species of amphibians (Pseudepidalea viridis, Hyla savignyi) in addition to five species of reptiles (Testudo graeca, Chamaeleo chamaeleon recticrista, Ophisops elegans, Lacerta media, Phoenicolacerta laevis) by replacing methyl violet 2B dye included in its composition with methyl violet 10B , where our results were compared with the values of previous studies, there is no any significant differences betw

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24

Roccatagliata, V., G. G. Sacco, E. Franciosini, and S. Randich. "The double population of Chamaeleon I detected by Gaia DR2." Astronomy & Astrophysics 617 (September 2018): L4. http://dx.doi.org/10.1051/0004-6361/201833890.

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Context. Chamaeleon I represents an ideal laboratory to study the cluster formation in a low-mass environment. Recently, two sub-clusters spatially located in the northern and southern parts of Chamaeleon I were found with different ages and radial velocities. Aims. In this Letter we report new insights into the structural properties, age, and distance of Chamaeleon I based on the astrometric parameters from Gaia data release 2 (DR2). Methods. We identified 140 sources with a reliable counterpart in the Gaia DR2 archive. We determined the median distance of the cluster using Gaia parallaxes an

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25

Lawson, Warrick A., and Lisa A. Crause. "Rotational and Candidate-Eclipsing-Binary Light Curves for Pre-Main-Sequence Stars in the Chamaeleon I Star-Forming Cloud." Publications of the Astronomical Society of Australia 26, no. 1 (2009): 31–36. http://dx.doi.org/10.1071/as08018.

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AbstractWe present the results of a photometric survey for variability in ten X-ray-emitting low-mass stars in the Chamaeleon region. Eight of the stars we observed are bona fide pre-main-sequence members of the ∼2 Myr-old Chamaeleon I star-forming cloud. The other two stars are young with high levels of relative X-ray emission, but with discordant proper motions they are probable non-members of the cloud. In six of the stars we monitored, periodic variations on timescales of 2.5–11.5 d were detected, that we ascribe to stellar rotation and the presence of cool starspots. Two other stars, CHXR

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26

Fielder, Samuel D., Helen Kirk, Michael M. Dunham, and Stella S. R. Offner. "An ALMA Search for Substructure and Fragmentation in Starless Cores in Orion B North." Astrophysical Journal 968, no. 1 (2024): 10. http://dx.doi.org/10.3847/1538-4357/ad3d56.

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Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 3 observations of 73 starless and protostellar cores in the Orion B North molecular cloud. We detect a total of 34 continuum sources at 106 GHz, and after comparisons with other data, four of these sources appear to be starless. Three of the four sources are located near groupings of protostellar sources, while one source is an isolated detection. We use synthetic observations of a simulation modeling a collapsing turbulent, magnetized core to compute the expected number of starless cores that should be detectable wi

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27

Cuadrado, Mariano, Isabel Molina-Prescott, and Luis Flores. "Comparison between tail and jugular venipuncture techniques for blood sample collection in common chameleons (Chamaeleo chamaeleon)." Veterinary Journal 166, no. 1 (2003): 93–97. http://dx.doi.org/10.1016/s1090-0233(02)00253-8.

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28

Blasco Ruiz, Manuel, J. L. Pérez-Botec, and J. M. Cabo. "Algunas reflexiones sobre el declive del camaleón común (Chamaeleo chamaeleon, L. 1758) en la Península Ibérica." Mediterránea. Serie de Estudios Biológicos, no. 17 (2000): 35–44. http://dx.doi.org/10.14198/mdtrra2000.17.04.

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29

Ouafa, Boudebia, Medila Ifriqya, and Toumi Ikram. "Evaluation of Biological Activities of Chamaeleo chamaeleon : A Reptile Used in Traditional Folk Medicine in Algeria." Journal of Biochemical Technology 13, no. 4 (2022): 15–19. http://dx.doi.org/10.51847/ed9gjaf2j7.

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30

Somody, Gergő, Zoltán Molnár, and Erika Lakatos. "Possibilities of rapid generation cycling of hemp (Cannabis sativa L.) for the stabilization of recessive traits." BIO Web of Conferences 125 (2024): 01012. http://dx.doi.org/10.1051/bioconf/202412501012.

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This study describes the development of a novel hemp germplasm using an accelerated breeding method. Two hemp varieties, ‘Balaton’ (green stem, very early female flowering) and ‘Chamaeleon’ (yellow stem, early maturing), were chosen for breeding. The breeding method involved crossing the varieties, manipulating light conditions to induce flowering, and performing artificial pollination. Yellow stem colour, a recessive trait from ‘Chamaeleon’, was successfully incorporated into the progeny within four generations in only twelve months overall. This demonstrates the effectiveness of the accelera

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31

Spezzi, L., N. L. J. Cox, T. Prusti, et al. "TheHerschelGould Belt Survey in Chamaeleon II." Astronomy & Astrophysics 555 (July 2013): A71. http://dx.doi.org/10.1051/0004-6361/201321444.

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32

Chen, Wen Ping, and J. A. Graham. "Duplicity Among Young Stars in Chamaeleon." International Astronomical Union Colloquium 135 (1992): 60–62. http://dx.doi.org/10.1017/s0252921100006114.

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AbstractWe present infrared imaging results of young stars in Cha I and II clouds that show either extended structure or a nearby neighboring star. Both regions appear to show high incidence rates of pairs. After excluding possible background stars, as judged from their brightness, color, or the local stellar surface number density, a frequency of 10% is deduced for binaries in Cha I with separations 2-5″, which is comparable to that in Taurus and to that of main sequence field stars.

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33

Sato, F., J. B. Whiteoak, R. E. Otrupcek, and M. Shimizu. "Cold HI Gas in the Chamaeleon I Dark Cloud Region." Publications of the Astronomical Society of Australia 9, no. 1 (1991): 145. http://dx.doi.org/10.1017/s1323358000025315.

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34

Schmidt, T. O. B., R. Neuhäuser, N. Vogt, A. Seifahrt, T. Roell та A. Bedalov. "Confirmation of the binary status of Chamaeleon Hα 2 – a very young low-mass binary in Chamaeleon". Astronomy & Astrophysics 484, № 2 (2008): 413–18. http://dx.doi.org/10.1051/0004-6361:20078381.

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35

Köhler, Rainer, and Wolfgang Brandner. "Multiplicity in T and OB Associations." Symposium - International Astronomical Union 200 (2001): 147–54. http://dx.doi.org/10.1017/s0074180900225163.

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The results of binary surveys among T Tauri stars in the T associations Taurus-Auriga and Chamaeleon, and in the OB association Scorpius-Centaurus are summarized, and implications on our understanding on the formation of binary and multiple systems are discussed.

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36

Ribas, Á., B. Merín, H. Bouy, et al. "Identification of transitional disks in Chamaeleon withHerschel." Astronomy & Astrophysics 552 (April 2013): A115. http://dx.doi.org/10.1051/0004-6361/201220960.

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37

López Martí, Belén, Francisco Jiménez-Esteban, Amelia Bayo, et al. "Proper motions of young stars in Chamaeleon." Astronomy & Astrophysics 556 (August 2013): A144. http://dx.doi.org/10.1051/0004-6361/201321217.

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38

Hughes, Joanne, and Patrick Hartigan. "Chamaeleon II - Distance determination and HR diagram." Astronomical Journal 104 (August 1992): 680. http://dx.doi.org/10.1086/116263.

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39

Lopez Martí, B., F. Jimenez Esteban, A. Bayo, D. Barrado, E. Solano, and C. Rodrigo. "Proper motions of young stars in Chamaeleon." Astronomy & Astrophysics 551 (February 19, 2013): A46. http://dx.doi.org/10.1051/0004-6361/201220128.

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40

Gahm, G. F., K. Lehtinen, P. Carlqvist, J. Harju, M. Juvela, and K. Mattila. "The threaded molecular clumps of Chamaeleon III." Astronomy & Astrophysics 389, no. 2 (2002): 577–88. http://dx.doi.org/10.1051/0004-6361:20020452.

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41

Gómez, M., and D. Mardones. "Near-Infrared Spectra of Chamaeleon I Stars." Astronomical Journal 125, no. 4 (2003): 2134–55. http://dx.doi.org/10.1086/368391.

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42

Toriseva, M., L. Bronfman, and K. Mattila. "C18O in the Chamaeleon I dark cloud." Astrophysics and Space Science 171, no. 1-2 (1990): 219–21. http://dx.doi.org/10.1007/bf00646851.

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43

Cuadrado, Mariano. "The influence of female size on the extent and intensity of mate guarding by males in Chamaeleo chamaeleon." Journal of Zoology 246, no. 3 (1998): 351–58. http://dx.doi.org/10.1111/j.1469-7998.1998.tb00165.x.

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44

Lev-Ari, Tidhar, Avichai Lustig, Hadas Ketter-Katz, Yossi Baydach, and Gadi Katzir. "Avoidance of a moving threat in the common chameleon (Chamaeleo chamaeleon): rapid tracking by body motion and eye use." Journal of Comparative Physiology A 202, no. 8 (2016): 567–76. http://dx.doi.org/10.1007/s00359-016-1106-z.

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45

McGregor, P. J., T. E. Harrison, J. H. Hough, and J. A. Bailey. "Infrared polarimetry in the Chamaeleon I dark cloud." Monthly Notices of the Royal Astronomical Society 267, no. 3 (1994): 755–65. http://dx.doi.org/10.1093/mnras/267.3.755.

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46

Belloche, A., F. Schuller, B. Parise, et al. "The end of star formation in Chamaeleon I?" Astronomy & Astrophysics 527 (February 14, 2011): A145. http://dx.doi.org/10.1051/0004-6361/201015733.

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47

Ikeda, Norio, Yoshimi Kitamura, Satoshi Takita, et al. "FAR-INFRARED IMAGING OBSERVATIONS OF THE CHAMAELEON REGION." Astrophysical Journal 745, no. 1 (2011): 48. http://dx.doi.org/10.1088/0004-637x/745/1/48.

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48

Luhman, K. L., J. C. Wilson, W. Brandner, et al. "Discovery of a Young Substellar Companion in Chamaeleon." Astrophysical Journal 649, no. 2 (2006): 894–99. http://dx.doi.org/10.1086/506517.

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49

Moeller, Holly V., and Matthew D. Johnson. "Preferential Plastid Retention by the Acquired PhototrophMesodinium chamaeleon." Journal of Eukaryotic Microbiology 65, no. 2 (2017): 148–58. http://dx.doi.org/10.1111/jeu.12446.

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50

Manara, C. F., D. Fedele, G. J. Herczeg, and P. S. Teixeira. "X-Shooter study of accretion in Chamaeleon I." Astronomy & Astrophysics 585 (January 2016): A136. http://dx.doi.org/10.1051/0004-6361/201527224.

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