…students urged to use experience from work studySeveral hundred students have completed the 2018 CSEC examination, and 300 of them have been selected to participate in the Region Four Department of Education’s Work Study Programme for 2018, which commences on Monday, June 18, 2018.REDO Tiffany Favourite-Harvey (at left) posing with Secondary Education Officers Loren Park and Carla Prescott-Mathews at (extreme right) from the Department of Education Region Four and work-study studentsActing Reginal Education Officer Tiffany Favourite-Harvey, in her address to the evidently eager students, urged them to use the experience and knowledge gained from the work study attachment to prepare themselves for the world of work.The 300 students would form two phases of students involved in work study, Favourite-Harvey disclosed, and some 46 agencies, organisations and businesses have come on board this programme this year.Favourite-Harvey stressed that it is the largest bunch of students to have ever been involved in the Region Four Work Study Programme. She added that while the average number over the years has been around 140 to 180, this year has seen 300 students coming on board.“While we are cognisant that many of you would be furthering your studies at the University of Guyana and other institutions, it is very important to note that demonstrating critical important qualities is pertinent in securing your dream job, or possibly getting your feet into the world of work. It is on this note that I urge you to inculcate attitudes and qualities that will hold you in good stead”, she told the students, who assembled at the Bladen Hall Multilateral School’s auditorium.The REDO reminded students that participation in the work study programme is no guarantee that the agency or company to which they would be sent would employ them after they would have completed their stint. She stressed that the experience would help the participants to better understand a number of issues that are important in the world of work.“Remember, you are not only representing yourself but, importantly, your school and the Department of Education, Region Four. Whatever you do will either give us praise or create embarrassment for us; so irrespective of how insignificant it may seem, do the right thing always,” she admonished.
TCI Premier blasts Opposition side for “slop” information, sets it straight in HOA Facebook Twitter Google+LinkedInPinterestWhatsAppProvidenciales, 23 Sept 2015 – It is National Youth Week and the PDM in a media statement says it’s Radio Show “Raising TCI” will return to the airwaves with a theme to honor young people. Opposition Leader, Sharlene Robinson explained about Youth guests that: “We will hear from them the challenges and what they feel can be done. We will also celebrate with the Miss Teen Organization….” Hon Robinson listed some challenges for young people including: “unemployment; under employment; depression; poverty; the growing inability to find their place or worth in their own country … lack of adult guidance; crimes; juvenile delinquency and improper facilities and programs…” but in her address, there was a charge for young people to, and again I quote: “…rise up and make your positive mark. You are required to contribute positively towards nation building. That is your duty and more so as you are the inheritors of what you build or destroy today.” National Youth Day is on Friday; it is a public holiday in the Turks and Caicos. Related Items:national youth week, Pdm, public holiday, radio show Facebook Twitter Google+LinkedInPinterestWhatsApp Recommended for you Only Doug and Ralph and Ruth can fit, that’s why TCI Country Leaders condemn vicious memes
“Bob quickly emerged as the candidate who would bring a powerful new perspective to our business,” says Christopher Coughlin, D&B’s current lead director, in a statement. “His track record of strategic leadership and innovation, combined with his ability to leverage a company’s core strengths and assets, uniquely position him to begin a new chapter in D&B’s history.”Replacing Carrigan will be IDG Enterprise CEO Michael Friedenberg, who will become CEO of IDG Communications U.S. David Hill, CEO of IDG International Publishing Services, will become president, overseeing international aspects of the media operation, among other responsibilities. Revenue at D&B was up one percent in the second quarter to $386.4 million, but flat for the first half at $767.4 million when compared to the same periods last year. Dun & Bradstreet Corp., the business data and marketing and risk management services provider, has selected Bob Carrigan as its new president, CEO and director. The appointment comes a month after Carrigan announced he was stepping down as CEO of IDG Communications Worldwide.Carrigan starts at D&B on October 7. He’ll be replacing Sara Mathew, who will be retiring from her position as the company’s chairman and CEO. Carrigan’s post at IDG Communications officially ends on September 30, at which point he’ll join the company’s board of directors.
, Astrophysical Journal , arXiv A trio of researchers with The University of Hong Kong, Academia Sinica Institute of Astronomy and Astrophysics in Taiwan and Northwestern University in the U.S., has come up with an alternative theory to explain how some stellar-mass black holes can grow bigger than others. In their paper published in The Astrophysical Journal Letters, Shu-Xu Yi, K.S. Cheng and Ronald Taam describe their theory and how it might work. Citation: Another way for stellar-mass black holes to grow larger (2018, August 17) retrieved 18 August 2019 from https://phys.org/news/2018-08-stellar-mass-black-holes-larger.html Since the initial detection of gravitational waves three years ago, five more detections have been observed—and five of the total have been traced back to emissions created by two stellar-mass black holes merging. The sixth was attributed to neutron stars merging. As part of their studies of such detections, space researchers have been surprised by the size of the stellar-mass black holes producing the gravity waves—they were bigger than other stellar-mass black holes. Their larger size has thus far been explained by the theory that they grew larger because they began their lives as stars that contained very small amounts of metal—stars with traces of metals would retain most of their mass because they produce weaker solar winds. In this new effort, the researchers suggest another possible way for stellar-mass black holes to grow larger than normal.The new theory starts out by noting that some supermassive black holes at the hearts of galaxies are surrounded by a disk of gas and dust. In such galaxies, there are often stars lying just outside the disk—stars that could evolve to become stellar-mass black holes. The researchers suggest that it is possible that sometimes, pairs of these stars wind up in the disk as they evolve into black holes. Such stellar-mass black holes would pull in material from the disk, causing them to grow larger. The researchers note that if such a scenario were to play out, it is also possible that the two merging stars could wind up with a synchronized spin resulting in a stellar-mass black hole that produces more gravity waves than if the spins had not been synchronized, making them easier for researchers to spot. More information: Shu-Xu Yi et al. The Growth of Stellar Mass Black Hole Binaries Trapped in the Accretion Disks of Active Galactic Nuclei, The Astrophysical Journal (2018). DOI: 10.3847/2041-8213/aac649 , On Arxiv: https://arxiv.org/abs/1805.07026AbstractAmong the four black hole (BH) binary merger events detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO), six progenitor BHs have masses greater than 20 M ⊙. The existence of such massive BHs suggests that extreme metal-poor stars are the progenitors. An alternative possibility, that a pair of stellar mass BHs each with mass ~7 M ⊙ increases to >20 M ⊙ via accretion from a disk surrounding a supermassive BH (SMBH) in an active galactic nucleus (AGN), is considered. The growth of mass of the binary and the transfer of orbital angular momentum to the disk accelerates the merger. Based on the recent numerical work of Tang et al., it is found that, in the disk of a low-mass AGN with mass ~106 M ⊙ and Eddington ratio >0.01, the mass of an individual BH in the binary can grow to >20 M ⊙ before coalescence, provided that accretion takes place at a rate more than 10 times the Eddington value. This mechanism predicts a new class of gravitational wave (GW) sources involving the merger of two extreme Kerr black holes associated with AGNs and a possible electromagnetic wave counterpart. Journal information: Astrophysical Journal Letters Explore further Image: Black hole bounty captured in the center of the Milky Way © 2018 Phys.org This artist’s impression shows a binary system containing a stellar-mass black hole called IGR J17091-3624, or IGR J17091 for short. The strong gravity of the black hole, on the left, is pulling gas away from a companion star on the right. This gas forms a disk of hot gas around the black hole, and the wind is driven off this disk. Credit: NASA/CXC/M.Weiss This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.