Results 221 to 230 of about 106,016 (255)

Population-based concordance of <i>Chlamydia trachomatis</i> genotypes between ocular and urogenital samples in Nauru. [PDF]

Microbiol Spectr
Lowry K, Apadinuwe S-C, Starr M, Star S, Lynch KD, Solomon AW, Cunningham P, Lambert S, Whiley D, Kaldor J, Vaz Nery S.   +10 more
europepmc   +1 more source

Improving Access to Specialty Care for Rural Children Using Enhanced Hearing Screening and Specialty Telehealth Follow-Up in Rural Kentucky Schools: Protocol for a Hybrid Effectiveness-Implementation Stepped Wedge, Cluster-Randomized Controlled Trial (Appalachian STAR Trial).

JMIR Res Protoc
Srinivasan T, Kleindienst Robler S, Turner E, Platt A, Arthur D, Prvu Bettger J, Lane H, Schuh Gebert M, Deshpande S, Schoenberg N, Bush ML, Emmett SD.   +11 more
europepmc   +1 more source

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

Fujimoto S, Ouchi M, Kohno K, Valentino F, Giménez-Arteaga C, Brammer G, Furtak L, Kohandel M, Oguri M, Pallottini A, Richard J, Zitrin A, Bauer F, Boylan-Kolchin M, Dessauges-Zavadsky M, Egami E, Finkelstein S, Ma Z, Smail I, Watson D, Hutchison T, Rigby J, Welch B, Ao Y, Bradley L, Caminha G, Caputi K, Espada D, Endsley R, Fudamoto Y, González-López J, Hatsukade B, Koekemoer A, Kokorev V, Laporte N, Lee M, Magdis G, Ono Y, Rizzo F, Shibuya T, Shimasaku K, Sun F, Toft S, Umehata H, Wang T, Yajima H.   +45 more
europepmc   +1 more source

Stellar collisions in young star clusters

, 2008
openaire   +1 more source

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Model based clustering for young star clusters

2018
Model based clustering is a method of fitting finite mixtures models to data in order to identify clusters. It is widely used in many fields and has a variety of applications,one of those is the identification of young star clusters. We will examine four different models multivariate Gaussian, t, Skew Normal and Skew t mixtures and a method that ...
openaire   +1 more source

Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang

Nature
The Cosmic Gems arc is among the brightest and highly magnified galaxies observed at redshift z ≈ 10.2 (ref. 1). However, it is an intrinsically ultraviolet faint galaxy, in the range of those now thought to drive the reionization of the Universe2–4 ...
A. Adamo, L. Bradley, E. Vanzella, A. Claeyssens, B. Welch, J. Diego, G. Mahler, M. Oguri, K. Sharon, Abdurro’uf, T. Hsiao, Xinfeng Xu, M. Messa, Augusto E Lassen, E. Zackrisson, G. Brammer, D. Coe, V. Kokorev, M. Ricotti, A. Zitrin, S. Fujimoto, A. Inoue, T. Resseguier, J. Rigby, Y. Jiménez-Teja, R. Windhorst, T. Hashimoto, Y. Tamura   +27 more
semanticscholar   +1 more source

Sexual health among adolescent and young adult cancer survivors: A scoping review from the Children's Oncology Group Adolescent and Young Adult Oncology Discipline Committee

Ca-A Cancer Journal for Clinicians, 2021
Brooke Cherven, Sharon L Bober, Kristin M Bingen   +2 more
exaly  

The Young Star Clusters in S106

1994
Near-infrared imaging of a 10 × 10 arcmin region of the S106 molecular cloud reveals two embedded clusters coinciding with peaks in the CO emission. By counting foreground stars seen towards the molecular cloud, the distance to S106 is found to be 1.2±0.2 kpc. Assuming a theoretical mass-luminosity relationship for pre-main sequence stars, we find that
openaire   +1 more source