• 제목/요약/키워드: PNE

검색결과 50건 처리시간 0.029초

INFRARED TWO-COLOR DIAGRAMS OF AGB STARS AND PLANETARY NEBULAE USING WISE DATA

  • Suh, Kyung-Won
    • 천문학회지
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    • 제51권5호
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    • pp.155-164
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    • 2018
  • We present various infrared two-color diagrams (2CDs) using WISE data for asymptotic giant branch (AGB) stars and Planetary Nebulae (PNe) and investigate possible evolutionary tracks. We use the sample of 5036 AGB stars, 660 post-AGB stars, and 2748 PNe in our Galaxy. For each object, we cross-identify the IRAS, AKARI, WISE, and 2MASS counterparts. To investigate the spectral evolution from AGB stars to PNe, we compare the theoretical model tracks of AGB stars and post-AGB stars with the observations on the IR 2CDs. We find that the theoretical dust shell model tracks can roughly explain the observations of AGB stars, post-AGB stars, and PNe on the various IR 2CDs. WISE data are useful in studying the evolution of AGB stars and PNe, especially for dim objects. We find that most observed color indices generally increase during the evolution from AGB stars to PNe. We also find that $Fe_{0.9}Mg_{0.1}O$ dust is useful to fit the observed WISE W3-W4 colors for O-rich AGB stars with thin dust shells.

일차성 야뇨증의 위험 요인 (Risk Factors of Primary Nocturnal Enuresis)

  • 이수진;양정안;유은선;서정완;이승주
    • Childhood Kidney Diseases
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    • 제4권1호
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    • pp.69-76
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    • 2000
  • 목 적 : 일차성 야뇨증의 병인론은 유전적 요인 외에 수면 요인, 야간 Arginine Vasopressin(AVP)분비 장애, 기능적 방광 미숙 등 주로 배뇨 반사의 성숙 지연이 논의되고 있으나 위험 요인에 대한 연구는 적었다. 이에 저자들은 소변을 충분히 가릴 나이인 5세 이후까지 야뇨증을 지속시킬 수 있는 위험 요인들을 분석하고자 하였다. 대상 및 방법 ;서울 목동지역 초등학교 1학년의 정기 신체 검사에서 야뇨증 설문지 조사를 통해 일차성 야뇨증으로 확인된 아동 20명과 이후 1년간 이화여자대학교 목동병원 소아과 외래에서 동일한 설문지 조사를 받은 6-7세의 일차성 야뇨증 아동 35명을 포함한 55명을 야뇨증군으로 하였고, 설문지 조사에서 야뇨증이 없었던 아동 221명을 대조군으로 하였다. 이중 야뇨증군 55명과 대조군 22명에서는 24시간 배뇨 일지를 기록하게 하였으며, 두 군사이에 유전적 요인, 심리적 요인, 발달 요인, 수면 요인, 일일 및 야간 수분 섭취량과 요량, 주간 배뇨 장애 및 일회 최대 요량 등을 비교분석 하였다. 결 과 : 1)부모의 야뇨증 병력은 야뇨증군에서 $20.0\%$로 대조군의 $2.7\%$에 비해 유의하게 많았다(P<0.05). 남녀비는 야뇨증군과 대조군에서 유의한 차이가 없었다. 2)출생 순서, 어머니의 직장 여부, 아동과 부모의 성격, 걷기 시작한 나이 및 학교 성적 두 군간에 유의한 차이가 없었다. 3) 잠에서 깨어나기 힘든 경우는 야뇨증군에서 $70.9\%$로 대조군의 $54.3\%$에 비해 유의하게 많았으나(P<0.05), 수면 시간은 차이가 없었다. 4) 야간 수분 섭취량은 야뇨증군에서 $330{\pm}158.2\;mL$로 대조군의 $235{\pm}129.5\;mL$에 비해 유의하게 많았고(P<0.05), 야간 요량은 야뇨증군에서 $390{\pm}61.5mL$로 대조군의 $140{\pm}43.2mL$에 비해 유의하게 많았다(P<0.05). 일일 수분 섭취량과 일일 요량은 두 군간에 유의한 차이가 없었다. 5) 일회 최대 요량은 야뇨증군에서 $107{\pm}35.9mL$로 대조군의 $236{\pm}41.3mL$에 비해 유의하게 적었다((P<0.05). 주간 배뇨 이상은 야뇨증군에서 $80.0\%$로 대조군의 $57.9\%$에 비해 유의하게 많았으며 주간 배뇨 횟수도 야뇨증군에서 $7.0{\pm}3.4$회로 대조군의 $5.4{\pm}1.6$회에 비해 유의하게 많았다(P<0.05). 결 론 :야뇨증은 유전적 요인을 비롯하여 성숙 지연과 관련된 수면 요인, 야간 다뇨, 방광 미숙 등이 관련될 것으로 생각된다. 야간 다뇨의 원인으로 야간 수분 섭취 과다가 관련되므로 치료의 일차 단계로 야간 수분 섭취 제한의 중요성이 강조되어야 한다고 생각된다.

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INVESTIGATION OF PAHs IN GALACTIC PLANETARY NEBULAE WITH THE AKARI/IRC AND THE SPITZER/IRS

  • Ohsawa, R.;Onaka, T.;Sakon, I.;Mori, T.I.;Yamamura, I.;Matsuura, M.;Kaneda, H.;Bernard-Salas, J.;Berne, O.;Joblin, C.
    • 천문학논총
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    • 제27권4호
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    • pp.259-260
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    • 2012
  • Polycyclic aromatic hydrocarbons (PAHs) in Galactic planetary nebulae (PNe) are investigated by means of the unidentified infrared (UIR) bands. Continuous near- to mid-infrared spectra of PNe are obtained with the AKARI/IRC and the Spitzer/IRS. All 19 PNe in the present study show prominent dust emissions and we investigate the variation in the intensity ratios among the UIR bands. The ionization fraction and the size distribution of PAHs in PNe are derived using the UIR band ratios. We find that the ionization fraction of PAHs in PNe is around 0.0-0.6 and that small PAHs are scarce. The present result indicates a systematic trend of the $3.4{\mu}m$ aliphatic feature to become weak as the PAH ionization fraction increases.

PLANETARY NEBULAE: NEW CHALLENGES IN THE 21ST CENTURY

  • KWOK SUN
    • 천문학회지
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    • 제38권2호
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    • pp.271-278
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    • 2005
  • Athough planetary nebulae (PNe) have been discovered for over 200 years, it was not until 30 years ago that we arrived at a basic understanding of their origin and evolution. Even today, with observations covering the entire electromagnetic spectrum from radio to X-ray, there are still many unanswered questions on their structure and morphology. In this review, we summarize recent theoretical and observational advances in PNe research, and discuss the roles of PNe in the chemical (atomic, molecular, and solid-state) enrichment of the galaxy and as tracers of the large scale structure of the Universe.

Pudendal nerve entrapment syndrome caused by ganglion cysts along the pudendal nerve

  • Kim, Young Je;Kim, Du Hwan
    • Journal of Yeungnam Medical Science
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    • 제38권2호
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    • pp.148-151
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    • 2021
  • Pudendal nerve entrapment (PNE) syndrome refers to the condition in which the pudendal nerve is entrapped or compressed. Reported cases of PNE associated with ganglion cysts are rare. Deep gluteal syndrome (DGS) is defined as compression of the sciatic or pudendal nerve due to a non-discogenic pelvic lesion. We report a case of PNE caused by compression from ganglion cysts and treated with steroid injection; we discuss this case in the context of DGS. A 77-year-old woman presented with a 3-month history of tingling and burning sensations in the left buttock and perineal area. Ultrasonography showed ganglion cystic lesions at the subgluteal space. Magnetic resonance imaging revealed cystic lesions along the pudendal nerve from below the piriformis to the Alcock's canal and a full-thickness tear of the proximal hamstring tendon. Aspiration of the cysts did not yield any material. We then injected steroid into the cysts, which resolved her symptoms. Steroid injection into a ganglion cyst should be considered as a treatment option for PNE caused by ganglion cysts.

Effects of pain neuroscience education on kinesiophobia in patients with chronic pain: a systematic review and meta-analysis

  • Kim, Hyunjoong;Lee, Seungwon
    • Physical Therapy Rehabilitation Science
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    • 제9권4호
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    • pp.309-317
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    • 2020
  • Objective: One of the treatment strategies for controlling chronic pain and preventing disability is patient education. Pain neuroscience education (PNE) has been proven to be effective in explaining the biological and physiological processes associated with pain experiences to patients. The purpose of this review is to investigate the effectiveness of PNE for kinesiophobia such as avoidance response in patients with chronic pain. Design: A systematic review and meta-analysis. Methods: MEDLINE, EMBASE, CINAHL, PEDro, and the Cochrane Central Register of controlled trials databases were searched through November 2020 and included a randomized controlled trials evaluating kinesiophobia in musculoskeletal patients with chronic pain. In 8 randomized controlled trial studies, 'Cochrane's risk of bias (RoB) tool was used for qualitative analysis, and results of post-intervention were analyzed through RevMan 5.4 for quantitative analysis. Results: For this review, 8 randomized controlled trials of 369 patients with chronic pain were selected for PNE. A systematic review and meta-analysis also included 8 randomized controlled trials. The effect on kinesiophobia was more effective than the control group (-0.86; 95% confidence interval [CI], -1.22 to -0.51; heterogeneity [χ2=21.18, df=7, I2=67%]; overall effect [Z=4.80]). In addition, the effect on pain was more effective than the control group (-0.53; 95% CI, -1.05 to -0.01; heterogeneity [χ2=47.42, df=7, I2=85%]; overall effect [Z=2.01]). Conclusions: The results of this review suggest that PNE and combined PNE have a positive effect on the improvement of pain and kinesiophobia in patients with chronic pain.

KINEMATICAL PROPERTIES OF PLANETARY NEBULAE WITH WR-TYPE NUCLEI

  • DANEHKAR, ASHKBIZ;STEFFEN, WOLFGANG;PARKER, QUENTIN A.
    • 천문학논총
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    • 제30권2호
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    • pp.163-167
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    • 2015
  • We have carried out integral field unit (IFU) spectroscopy of $H{\alpha}$, [$N{\small{II}}$] and [$O{\small{III}}$] emission lines for a sample of Galactic planetary nebulae (PNe) with Wolf-Rayet (WR) stars and weak emission-line stars (wels). Comparing their spatially-resolved kinematic observations with morpho-kinematic models allowed us to disentangle their three-dimensional gaseous structures. Our results indicate that these PNe have axisymmetric morphologies, either bipolar or elliptical. In many cases the associated kinematic maps for the PNe around hot central stars also reveal the presence of so-called fast low-ionization emission regions.

고성능 장비의 정밀도 향상을 위한 새로운 D/A 설계기법 (New D/A Design Method for Improving Accuracy in High-Performance Test Equipment)

  • 김형중;채수용
    • 전력전자학회:학술대회논문집
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    • 전력전자학회 2018년도 전력전자학술대회
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    • pp.308-309
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    • 2018
  • This paper proposes new D/A(Digital to Analog) Design method for improving accuracy in high-performance test equipment. The proposed new D/A design can improve accuracy of the equipment even with low-resolution D/A converters. The validity of proposed D/A design is verified by analysis and experiment.

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한방병원 야뇨 환아의 후향적 연구 (A follow-up study of enuretic children)

  • 장규태;김장현;오주영
    • 대한한방소아과학회지
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    • 제18권1호
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    • pp.179-191
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    • 2004
  • Objective: The aim of this study was to investigate enuretic children attending oriental hospital and classify subtypes and evaluate possible factors that enhance or hamper of continence. Methods: Children attending kyeongju dongguk oriental hospital pediatrics between January 2000 and December 2003 with chief complaint of nocturnal enuresis were enrolled. The data of present symptoms and improvement progress was collected via telephone interviews with their parents. Results: The total number of children was 61. 32 of them were male and 29 female. Sex ratio was 1.1:1. Patient under 6 years of age was 68.8%. Using acupuncture, acupressure or chimsband with herb medicine, treatment frequency was increased. Patients with nocturnal enuresis(NE) was 48, and primary nocturnal enuresis(PNE) 39, secondary (SNE) 9. 13 was impossible to diagnose. The ratio of male to female was 1:1.09. PNE was 4 times as many as SNE. Male was predominent in PNE, and female in SNE. In the progress of PNE, male and female were similiar. but SNE, male was all cured, female remained 50%. And elapsed time of male to improve was longer than that of female. In the progress of improvement, many parents mentioned that their child was improved spontaneously regardless of subtype. Conclusion: We consider age, sex distinction, subtype, bladder symptoms, frequency, time of progress as influencing factor of prognosis, but failed to verify significance. To develop guideline of NE and find influencing factor of prognosis, more prospective study through taking history carefully and using questionnaire is needed.

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NEAR-INFRARED PAH FEATURES IN GALACTIC PLANETARY NEBULAE

  • Ohsawa, R.;Onaka, O.;Sakon, I.;Mori, T. I.;Kaneda, H.;Matsuura, M.
    • 천문학논총
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    • 제32권1호
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    • pp.87-91
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    • 2017
  • Polycyclic aromatic hydrocarbons (PAHs) are considered to be carriers of the unidentified infrared bands, which are ubiquitously observed in the Universe. PAHs are mainly formed around evolved carbon-rich stars and injected into interstellar space. Planetary nebulae (PNe), a late stage of low- and intermediate stellar mass evolution, are suitable objects to investigate the formation and evolution of PAHs. The shortest PAH feature is located in $3.3{\mu}m$, which is important to examine the excitation and size distribution of PAHs. While the number of samples had been limited before, the high sensitivity of AKARI /IRC has drastically increased the number of samples. We obtained the $2-5{\mu}m$ spectra of Galactic PNe with AKARI /IRC and compiled a near-infrared spectral catalog, containing 73 PNe. We investigate the detection rate and the evolution of the PAH features. The characteristics of the catalog are illustrated and the origin of the evolution of the PAH features is discussed.