ALBERT

Description: Modern strains of Mycobacterium tuberculosis from the Americas are closely related to those from Europe, supporting the assumption that human tuberculosis was introduced post-contact. This notion, however, is incompatible with archaeological evidence of pre-contact tuberculosis in the New World. Comparative genomics of modern isolates suggests that M. tuberculosis attained its worldwide distribution following human dispersals out of Africa during the Pleistocene epoch, although this has yet to be confirmed with ancient calibration points. Here we present three 1,000-year-old mycobacterial genomes from Peruvian human skeletons, revealing that a member of the M. tuberculosis complex caused human disease before contact. The ancient strains are distinct from known human-adapted forms and are most closely related to those adapted to seals and sea lions. Two independent dating approaches suggest a most recent common ancestor for the M. tuberculosis complex less than 6,000 years ago, which supports a Holocene dispersal of the disease. Our results implicate sea mammals as having played a role in transmitting the disease to humans across the ocean.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4550673/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4550673/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Bos, Kirsten I -- Harkins, Kelly M -- Herbig, Alexander -- Coscolla, Mireia -- Weber, Nico -- Comas, Inaki -- Forrest, Stephen A -- Bryant, Josephine M -- Harris, Simon R -- Schuenemann, Verena J -- Campbell, Tessa J -- Majander, Kerttu -- Wilbur, Alicia K -- Guichon, Ricardo A -- Wolfe Steadman, Dawnie L -- Cook, Della Collins -- Niemann, Stefan -- Behr, Marcel A -- Zumarraga, Martin -- Bastida, Ricardo -- Huson, Daniel -- Nieselt, Kay -- Young, Douglas -- Parkhill, Julian -- Buikstra, Jane E -- Gagneux, Sebastien -- Stone, Anne C -- Krause, Johannes -- 098051/Wellcome Trust/United Kingdom -- AI090928/AI/NIAID NIH HHS/ -- MC_U117581288/Medical Research Council/United Kingdom -- R01 AI090928/AI/NIAID NIH HHS/ -- Medical Research Council/United Kingdom -- England -- Nature. 2014 Oct 23;514(7523):494-7. doi: 10.1038/nature13591. Epub 2014 Aug 20.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉1] Department of Archaeological Sciences, University of Tubingen, Ruemelinstrasse 23, 72070 Tubingen, Germany [2]. ; 1] School of Human Evolution and Social Change, Arizona State University, PO Box 872402, Tempe, Arizona 85287-2402, USA [2]. ; 1] Department of Archaeological Sciences, University of Tubingen, Ruemelinstrasse 23, 72070 Tubingen, Germany [2] Center for Bioinformatics, University of Tubingen, Sand 14, 72076 Tubingen, Germany [3]. ; 1] Department of Medical Parasitology and Infection Biology, Swiss Tropical and Public Health Institute, Socinstrasse 57, 4002 Basel, Switzerland [2] University of Basel, Petersplatz 1, CH-4003 Basel, Switzerland [3]. ; Center for Bioinformatics, University of Tubingen, Sand 14, 72076 Tubingen, Germany. ; 1] Genomics and Health Unit, FISABIO-Public Health, Avenida Cataluna 21, 46020 Valencia, Spain [2] CIBER (Centros de Investigacion Biomedica en Red) in Epidemiology and Public Health, Instituto de Salud Carlos III, C/ Monforte de Lemos 3-5, Pabellon 11, Planta 0, 28029 Madrid, Spain. ; Department of Archaeological Sciences, University of Tubingen, Ruemelinstrasse 23, 72070 Tubingen, Germany. ; Pathogen Genomics, The Wellcome Trust Sanger Institute, Wellcome Trust Genome Campus, Hinxton, Cambridge CB10 1SA, UK. ; Department of Archaeology, University of Cape Town, Private Bag X1, Rondebosch, 7701, South Africa. ; School of Human Evolution and Social Change, Arizona State University, PO Box 872402, Tempe, Arizona 85287-2402, USA. ; CONICET, Laboratorio de Ecologia Evolutiva Humana (FACSO, UNCPBA), Departamento de Biologia (FCEyN, UNMDP), Calle 508 No. 881 (7631), Quequen, Argentina. ; Department of Anthropology, University of Tennessee, 250 South Stadium Hall, Knoxville, Tennessee 37996, USA. ; Department of Anthropology, Indiana University, 701 East Kirkwood Avenue, Bloomington, Indiana 47405-7100, USA. ; 1] Molecular Mycobacteriology, Forschungszentrum Borstel, Parkallee 1, 23845 Borstel, Germany [2] German Center for Infection Research, Forschungszentrum Borstel, Parkallee 1, 23845 Borstel, Germany. ; McGill International TB Centre, McGill University, 1650 Cedar Avenue, Montreal H3G 1A4, Canada. ; Biotechnology Institute, CICVyA-INTA Castelar, Dr. Nicolas Repetto y De Los Reseros S/N, (B1686IGC) Hurlingham, Buenos Aires, Argentina. ; Instituto de Investigaciones Marinas y Costeras (CONICET-UNMdP), Facultad de Ciencias Exactas y Naturales, Universidad Nacional de Mar del Plata, San Luis 1722, Mar del Plata 7600, Argentina. ; 1] Department of Medicine, Imperial College, London W2 1PG, UK [2] Division of Mycobacterial Research, MRC National Institute for Medical Research, Mill Hill, London NW7 1AA, UK. ; 1] Department of Medical Parasitology and Infection Biology, Swiss Tropical and Public Health Institute, Socinstrasse 57, 4002 Basel, Switzerland [2] University of Basel, Petersplatz 1, CH-4003 Basel, Switzerland. ; 1] Department of Archaeological Sciences, University of Tubingen, Ruemelinstrasse 23, 72070 Tubingen, Germany [2] Senckenberg Centre for Human Evolution and Palaeoenvironment, University of Tubingen, Tubingen 72070, Germany [3] Max Planck Institute for Science and History, Khalaische Strasse 10, 07745 Jena, Germany.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25141181" target="_blank"〉PubMed〈/a〉

Description: We measured carbonyl sulfide (COS) in air extracted from ice core samples from the West Antarctic Ice Sheet (WAIS) Divide, Antarctica, with the deepest sample dated to 54,300 years before present. These are the first ice core COS measurements spanning the last glacial maximum (LGM), the last glacial/interglacial transition, and the early Holocene. The WAIS Divide measurements from the LGM and the last transition are the first COS measurements in air extracted from full clathrate (bubble-free) ice. This study also includes new COS measurements from Taylor Dome, Antarctica, including some in bubbly glacial-ice that are concurrent with the WAIS Divide data from clathrate glacial-ice. COS hydrolyzes in ice core air bubbles and the recovery of an atmospheric record requires correcting for this loss. The data presented here suggest that the in situ hydrolysis of COS is significantly slower in clathrate ice than in bubbly ice. The clathrate-ice measurements are corrected for the hydrolysis loss during the time spent as bubbly ice only. The corrected WAIS Divide record indicates that atmospheric COS was 250-300 ppt during the LGM and declined by 80 – 100 ppt during the last glacial/interglacial transition to a minimum at 160-210 ppt at the beginning of the Holocene. This decline was likely caused by an increase in the gross primary productivity of terrestrial plants, with a possible contribution from a reduction in ocean sources. COS levels were above 300 ppt in the late Holocene, indicating that large changes in the COS biogeochemical cycle occurred during the Holocene.

Description: Author(s): S. Campbell, T. J. G. Apollaro, C. Di Franco, L. Banchi, A. Cuccoli, R. Vaia, F. Plastina, and M. Paternostro [Phys. Rev. A 84, 052316] Published Tue Nov 15, 2011

Description: αv integrins on mesenchymal cells regulate skeletal and cardiac muscle fibrosis Nature Communications, Published online: 24 October 2017; doi:10.1038/s41467-017-01097-z The mechanisms underlying tissue fibrosis are unclear. The authors show that mesenchymal cells expressing PDGFRβ mediate fibrosis in skeletal muscle and heart via a mechanism involving αv integrin, and that inhibitors of αv integrins attenuate fibrotic responses in mice.

Description: We summarize the results of a 20-yr campaign to study the light curves of BK Lyn, a nova-like star strangely located below the 2 to 3 h orbital-period gap in the family of cataclysmic variables (CVs). Two apparent superhumps dominate the nightly light curves, with periods 4.6 per cent longer, and 3.0 per cent shorter, than the orbital period. The first appears to be associated with the star's brighter states ( V  ~ 14), while the second appears to be present throughout and becomes very dominant in the low state ( V  ~ 15.7). It is plausible that these arise, respectively, from a prograde apsidal precession and a retrograde nodal precession of the star's accretion disc. Starting in the year 2005, the star's light curve became indistinguishable from that of a dwarf nova – in particular, that of the ER UMa subclass. No such clear transition has ever been observed in a CV before. Reviewing all the star's oddities, we speculate: (a) BK Lyn is the remnant of the probable nova on 101 December 30, and (b) it has been fading ever since, but it has taken ~2000 yr for the accretion rate to drop sufficiently to permit dwarf-nova eruptions. If such behaviour is common, it can explain other puzzles of CV evolution. One : why the ER UMa class even exists (because all members can be remnants of recent novae). Two : why ER UMa stars and short-period nova-likes are rare (because their lifetimes, which are essentially cooling times, are short). Three : why short-period novae all decline to luminosity states far above their true quiescence (because they are just getting started in their post-nova cooling). Four : why the orbital periods, accretion rates and white dwarf temperatures of short-period CVs are somewhat too large to arise purely from the effects of gravitational radiation (because the unexpectedly long interval of enhanced post-nova brightness boosts the mean mass-transfer rate). And maybe even five : why very old, post-period-bounce CVs are hard to find (because the higher mass-loss rates have ‘burned them out’). These are substantial rewards in return for one investment of hypothesis: that the second parameter in CV evolution, besides orbital period, is time since the last classical-nova eruption .