| 2501. |
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| 2502. |
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| 2503. |
- Jansson, C, et al.
(author)
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Relation between gastroesophageal reflux symptoms and socioeconomic factors : a population-based study (the HUNT Study)
- 2007
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In: Clinical Gastroenterology and Hepatology. - : Elsevier BV. - 1542-3565 .- 1542-7714. ; 5:9, s. 1029-1034
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Journal article (peer-reviewed)abstract
- BACKGROUND & AIMS: Gastroesophageal reflux constitutes a major public health problem in the Western world. Few population-based studies have addressed socioeconomic factors in relation to reflux. METHODS: We conducted a case-control study based on 2 health surveys performed in the Norwegian county of Nord-Trondelag in 1984-1986 and 1995-1997, respectively. Reflux was assessed in the second survey, comprising 65,333 participants representing 70% of the county's adult population. Among 58,596 persons responding to questions regarding reflux symptoms, 3153 persons reporting severe symptoms represented the cases, and 40,210 persons without symptoms represented the controls. Data collected in questionnaires included socioeconomic status (SES) based on occupation, education, and material deprivation; family situation; and potential confounders. Odds ratios (ORs) with 95% confidence intervals (CIs) were estimated from unconditional logistic regression in crude models and models adjusted for age, sex, smoking, and body mass. RESULTS: The risk of reflux increased with decreasing levels of SES based on occupation, education, and material deprivation. Increased risks of reflux were seen among unskilled laborers (OR, 1.6; 95% CI, 1.3-2.0), skilled laborers (OR, 1.4; 95% CI, 1.1-1.7), and self-employed and farmers (OR, 1.3; 95% CI, 1.1-1.6). A 1.9-fold (95% CI, 1.7-2.2) increased risk of reflux was observed among persons with low education, compared with highly educated persons. Reflux was more common among materially deprived persons (OR, 3.4; 95% CI, 2.9-4.1). The results were similar in crude and adjusted models. CONCLUSIONS: This large population-based study reveals a link between low SES and reflux symptoms that is not explained by the known risk factors of smoking or obesity. This finding deserves further research.
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| 2504. |
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| 2505. |
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| 2506. |
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| 2507. |
- Jansson, C, et al.
(author)
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The prevalence of symptoms possibly related to the climacteric in pre- and postmenopausal women in Link÷ping, Sweden
- 2003
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In: Maturitas. - 0378-5122 .- 1873-4111. ; 45:2, s. 129-135
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Journal article (peer-reviewed)abstract
- Background: Some extragenital symptoms have been suggested to be associated with the menopause and thus to be affected by estrogen status. In such case extragenital symptoms may be more frequent in postmenopausal women without hormone replacement therapy (HRT) than in premenopausal women or women using HRT. Objective: To assess if the prevalence of a number of extragenital symptoms is higher in postmenopausal women without than with HRT, or in premenopausal women of the same age. Material and methods: All women aged 53 and 54 years in the community of Link÷ping (n=1760) were sent a validated questionnaire about use of HRT, time since last menstruation and about different extragenital symptoms. Results: 1298 (73.8%) women answered the questionnaire and answers from 1180 (67%) women were possible to analyze. Postmenopausal women woke up significantly more often during night than premenopausal, and those without HRT often due to hot flushes and sweating. Women with HRT reported more muscular pain than the others. We found no other significant difference in prevalence of extragenital symptoms between the three groups of women. Conclusions: Sleeping disorders, arthralgia, xerophthalmia, xerostomia and dry skin are not more prevalent in 53 and 54 years old postmenopausal women without HRT than in women with HRT or in premenopausal women of the same age. It may still be that some of these symptoms are related to estrogen deficiency, but do not develop until some years after menopause. It may also be that women with the most severe symptoms decided to use HRT and thereby decreased symptoms to the same level as in non-users. ⌐ 2003 Elsevier Science Ireland Ltd. All rights reserved.
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| 2508. |
- Jansson, D. S., et al.
(author)
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Brachyspira hyodysenteriae and other strongly beta-haemolytic and indole-positive spirochaetes isolated from mallards (Anas platyrhynchos)
- 2004
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In: Journal of Medical Microbiology. - : Microbiology Society. - 0022-2615 .- 1473-5644. ; 53:4, s. 293-300
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Journal article (peer-reviewed)abstract
- The aims of the current study were to collect intestinal spirochaetes (genus Brachyspira) from farmed and wild mallards (Anas platyrhynchos) and to identify and classify those isolates that phenotypically resembled Brachyspira hyodysenteriae, an enteric pathogen of pigs. The isolation rate of Brachyspira spp. was high from both farmed (93%) and wild mallards (78%). In wild mallards, it appeared that Brachyspira spp. were more likely to be found in migratory birds (multivariate analysis: RR = 1(.)8, 95% Cl 1(.)1-3(.)1) than in mallards sampled in a public park. Pure cultures of putative B. hyodysenteriae were obtained from 22 birds. All five isolates from farmed mallards and ten randomly selected isolates with this phenotype were used for further studies. All isolates from farmed mallards and two of the isolates from wild mallards were PCR-positive for the tlyA gene of B. hyodysenteriae. Two isolates from farmed mallards were selected for pulsed field gel electrophoresis (PFGE) and randomly amplified polymorphic DNA (RAPD) analysis. These isolates clustered with the type and reference strains of B. hyodysenteriae. 16S rDNA sequence analysis performed on 11 of the strains showed that they were all closely related to each other and to the B. hyodysenteriae-Brachyspira intermedia cluster. Three of the mallard isolates had 16S rDNA sequences that were identical to those of B. hyodysenteriae strains R1 and NIV-1 previously isolated from common rheas (Rhea americana). To conclude, the isolates from farmed mallards and two isolates from wild mallards were classified as B. hyodysenteriae based on the factthat they could not be differentiated by any of the applied methods from type, reference and field strains of B. hyodysenteriae. The remaining isolates could not be assigned irrefutably to any of the presently recognized Brachyspira species. These results point to a broader host spectrum of B. hyodysenteriae than is generally recognized, and to the presence in mallards of strongly haemolytic and indole-producing spirochaetes that possess many, but not all, of the currently recognized characteristics of B. hyodysenteriae.
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| 2509. |
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| 2510. |
- Jencson, Jacob E., et al.
(author)
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AT 2019qyl in NGC 300 : Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary
- 2021
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In: Astrophysical Journal. - : American Astronomical Society. - 0004-637X .- 1538-4357. ; 920:2
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Journal article (peer-reviewed)abstract
- Nova eruptions, thermonuclear explosions on the surfaces of white dwarfs (WDs), are now recognized to be among the most common shock-powered astrophysical transients. We present the early discovery and rapid ultraviolet (UV), optical, and infrared (IR) temporal development of AT 2019qyl, a recent nova in the nearby Sculptor Group galaxy NGC 300. The light curve shows a rapid rise lasting ≲1 day, reaching a peak absolute magnitude of MV = −9.2 mag and a very fast decline, fading by 2 mag over 3.5 days. A steep dropoff in the light curves after 71 days and the rapid decline timescale suggest a low-mass ejection from a massive WD with MWD ≳ 1.2 M⊙. We present an unprecedented view of the early spectroscopic evolution of such an event. Three spectra prior to the peak reveal a complex, multicomponent outflow giving rise to internal collisions and shocks in the ejecta of an He/N-class nova. We identify a coincident IR-variable counterpart in the extensive preeruption coverage of the transient location and infer the presence of a symbiotic progenitor system with an O-rich asymptotic-giant-branch donor star, as well as evidence for an earlier UV-bright outburst in 2014. We suggest that AT 2019qyl is analogous to the subset of Galactic recurrent novae with red-giant companions such as RS Oph and other embedded nova systems like V407 Cyg. Our observations provide new evidence that internal shocks between multiple, distinct outflow components likely contribute to the generation of the shock-powered emission from such systems.
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