• Title/Summary/Keyword: Mass Scaling

검색결과 137건 처리시간 0.024초

Galactic Globular and Open Clusters in the Sloan Digital Sky Survey. III. Horizontal Branch Stars and Mass Loss in NGC 6791

  • Yu, Hyein;An, Deokkeun;Chung, Chul
    • 천문학회보
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    • 제39권1호
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    • pp.61.2-61.2
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    • 2014
  • We present a set of fiducial sequences of horizontal-branch stars in bright Galactic globular clusters, which have previously been observed in the Sloan Digital Sky Survey (SDSS). We derive fiducial lines on color-magnitude diagrams in multiple color indices (g - r, g - i, g - z, and u - g), after rejecting foreground and background objects as well as RR Lyrae variables utilizing these color indices. We compare our fiducial sequences with model predictions from Yonsei-Yale evolutionary tracks and BaSel spectral libraries, and find a satisfactory agreement between them in terms of their color-magnitude relations, except in u - g. We also compare theoretical models to color-magnitude diagrams of two open clusters (M67 and NGC 6791). Based on our best available cluster distance and reddening, we find that the mass of red clump (RC) stars in NGC 6791 is about a factor of two smaller than an earlier estimate from the application of asteroseismic scaling relations for solar-like oscillations. The smaller RC mass implies an enhanced mass loss along the red giant branch, which is in accordance with other compelling evidences found in this metal-rich system. Our estimated luminosity of RC stars in NGC 6791 is about 0.2 mag fainter than in earlier investigations based on solar-metallicity calibrations, and results in ~10% reduction in the RC-based distance estimation, when applied to metal-rich systems such as in the Galactic bulge.

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Relation between Black Hole Mass and Bulge in Hard X-ray selected Type 1 AGNs

  • Son, Suyeon;Kim, Minjin;Barth, Aaron J.;Ho, Luis C.
    • 천문학회보
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    • 제45권1호
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    • pp.62.1-62.1
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    • 2020
  • We present a scaling relation between black hole (BH) mass and bulge luminosity for 35 nearby (z<0.1) type 1 active galaxies, selected from the 70-month Swift-BAT X-ray source catalog. Thanks to the unbiased selection and proximity of the parent sample, our sample is suitable to study the physical connection between central black holes and host galaxies. We use the F814W images obtained with the Advanced Camera for Surveys on Hubble Space Telescope, to perform the imaging decomposition with GALFIT. With a careful treatment on the PSF model, we measure the I-band bulge brightness robustly. In combination with the BH mass estimated from a single-epoch spectroscopic data, we present the correlation between BH mass and bulge luminosity of the target AGNs. We demonstrate that our sample marginally lies off from the M(BH)-L(bulge) relation of inactive galaxies. We discuss possible physical origins of this discrepancy. Finally, we present how the relation depends on the photometric properties of AGNs and host galaxies, which may provide an useful insight on the co-evolution between BHs and host galaxies.

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Investigating the cosmic evolution of the black hole mass-bulge luminosity scaling relation

  • Park, Daeseong;Woo, Jong-Hak;Treu, Tommaso;Bennert, Vardha N.;Malkan, Matthew A.;Auger, Matthew W.
    • 천문학회보
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    • 제38권2호
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    • pp.42.2-42.2
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    • 2013
  • We investigate the cosmic evolution of the black hole mass-bulge luminosity relation with a sample of 52 moderate-luminosity AGNs at $z{\simeq}0.36$ and $z{\simeq}0.57$, corresponding to look-back times of 4 and 6 Gyrs. By employing robust multi-component spectral and structural decomposition methods to the obtained high-quality Keck spectra and high-resolution HST images, black hole masses ($M_{BH}$) are estimated from the Hbeta broad emission line with the 5100A nuclear luminosity, and bulge luminosities ($L_{bul}$) are derived from the surface photometry. Based on these consistent measurements, we constrain the redshift evolution of the $M_{BH}-L_{bul}$ relation by performing the Monte Carlo simulations designed to account for selection effects. We provide implications of our results in terms of the black hole-galaxy co-evolution and discuss possible bulge growth mechanisms.

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다공도 및 팽창파의 영향을 고려한 BLEED 경계조건 수치 모델링의 정확도 향상 연구 (ACCURACY IMPROVEMENT OF THE BLEED BOUNDARY CONDITION WITH THE EFFECTS OF POROSITY VARIATIONS AND EXPANSION WAVES)

  • 김광현;최요한;김종암
    • 한국전산유체공학회지
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    • 제21권1호
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    • pp.94-102
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    • 2016
  • The present paper deals with accuracy improvement of a bleed boundary condition model used to improve the performance of supersonic inlets. In order to accurately predict the amount of bleed mass flow rates, this study performs a scaling of sonic flow coefficient data for 90-degree bleed holes in consideration of Prandtl-Meyer expansion theory. Furthermore, it is assumed that porosity varies with stream-wise location of the porous bleed plate to accurately predict downstream boundary layer profiles. The bleed boundary condition model is demonstrated through Computational Fluid Dynamics(CFD) simulations of bleed flows on a flat plate with/without an oblique shock. As a result, the bleed model shows the improved accuracy of bleed mass rates and downstream boundary layer profiles.

KYDISC program: The Impact of Mergers on the Evolution of Galaxies

  • Oh, Sree
    • 천문학회보
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    • 제42권1호
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    • pp.30.1-30.1
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    • 2017
  • In the hope to detect low-surface brightness features (${\mu}_{r^{\prime}}{\sim}27\;mag\;arcsec^{-2}$), we carried out KASI-Yonsei Deep Imaging Survey for Clusters (KYDISC) targeting 14 local clusters at 0.016 < z < 0.145 using Magellan/IMACS telescope and CFHT/MegaCam. Out of 1450 cluster galaxies, 18% of galaxies show the signatures of galaxy mergers. We explore merger-driven changes from various point-of-view. We first examine color-magnitude relations, and find that galaxies related to recent mergers are populated more on blue color than their counterparts. Besides, we find the extremely low frequency of mergers on low-mass red-sequence galaxies, suggesting a migration of red galaxies into the green-valley region through merger-driven star-formation. We also study the mass-size relation of our sample, finding a larger galaxy size in galaxies related to recent mergers. Our results suggest that mergers can simultaneously change properties of galaxies, making outliers on galactic scaling relations.

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준정적 충돌해석을 통한 선박충돌방공호의 방호능력평가 (A Protection Capacity Evaluation of Vessel Protective Structures by Quasi-Static Collision Analysis)

  • 이계희
    • 한국전산구조공학회논문집
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    • 제24권6호
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    • pp.691-697
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    • 2011
  • 본 연구에서는 방호공의 최대방호능력을 산정하기 위하여 선박충돌방호공과 선박을 수치적으로 모델링하고 준정적해석으로 충돌해석을 수행하였다. 방호공은 구조물의 비선형 거동과 지반의 지지효과 및 인발을 고려하여 모델링되었다. 충돌선박은 비선형거동이 집중되는 선수부분을 정밀하게 모델링하고 효율적인 해석을 위해 mass scaling기법을 사용하였다. 동일한 해석모델에 대하여 동적해석을 추가적으로 수행하여 두 해석방법의 차이점과 효율성을 평가하였다. 선박과 방호공의 에너지소산곡선을 바탕으로 충돌선박이 교량하부구조에 충돌력을 전달되는 시점을 추정하고, 이를 바탕으로 대상선박의 최대충돌허용속도를 산정하였다. 이러한 추정방법이 방호공의 에너지소산한계를 명확히 판단할 수 있어 공학적으로 효율적인 산정방법임을 보였다.

Experimental and numerical FEM of woven GFRP composites during drilling

  • Abd-Elwahed, Mohamed S.;Khashaba, Usama A.;Ahmed, Khaled I.;Eltaher, Mohamed A.;Najjar, Ismael;Melaibari, Ammar;Abdraboh, Azza M.
    • Structural Engineering and Mechanics
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    • 제80권5호
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    • pp.503-522
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    • 2021
  • This paper investigates experimentally and numerically the influence of drilling process on the mechanical and thermomechanical behaviors of woven glass fiber reinforced polymer (GFRP) composite plate. Through the experimental analysis, a CNC machine with cemented carbide drill (point angles 𝜙=118° and 6 mm diameter) was used to drill a woven GFRP laminated squared plate with a length of 36.6 mm and different thicknesses. A produced temperature during drilling "heat affected zone (HAZ)" was measured by two different procedures using thermal IR camera and thermocouples. A thrust force and cutting torque were measured by a Kistler 9272 dynamometer. The delamination factors were evaluated by the image processing technique. Finite element model (FEM) has been developed by using LS-Dyna to simulate the drilling processing and validate the thrust force and torque with those obtained by experimental technique. It is found that, the present finite element model has the capability to predict the force and torque efficiently at various drilling conditions. Numerical parametric analysis is presented to illustrate the influences of the speeding up, coefficient of friction, element type, and mass scaling effects on the calculated thrust force, torque and calculation's cost. It is found that, the cutting time can be adjusted by drilling parameters (feed, speed, and specimen thickness) to control the induced temperature and thus, the force, torque and delamination factor in drilling GFRP composites. The delamination of woven GFRP is accompanied with edge chipping, spalling, and uncut fibers.

터널 화재시 종류식 환기가 연소율 변화에 미치는 영향에 관한 실험적 연구 (An Experimental Study on the Effect of Longitudinal Ventilation on the Variation of Burning Rate in Tunnel Fires)

  • 양승신;김성찬;유홍선
    • 터널과지하공간
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    • 제15권1호
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    • pp.55-60
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    • 2005
  • 본 연구는 터널내 화재 발생시 종류식 환기가 연소율 변화에 미치는 영향을 파악하기 위하여 Froude scaling에 의해 1/20크기로 축소한 모형화재 실험을 수행하였다. 화원으로는 $8.5cm{\sim}14.5cm$의 메탄올을 사용하였으며 발열량은 $3.57{\sim}10.95kW$이다. 연소율은 로드셀을 이용하여 산출하였고, 연기거동을 파악하기 위하여 K형 열전대를 이용하여 온도분포를 측정하였다. 풍동은 터널의 한쪽부분과 연결하였고, 터널 공간의 배연속도를 제어하기 위하여 풍동의 전압을 조절하였다. 메탄올 화재인 경우 배연속도가 증가할수록 냉각효과로 인하여 연소율은 감소하였으며, 또한 같은 무차원속도(V)일때 화원 크기가 커짐에 따라 연소율은 감소하였다.

터널 화재시 배연속도가 연소율변화에 미치는 실험적 연구 - Heptane 풀화재 경우 (An Experimental Study on the Ventilation velocity of the Variation of Burning rate in Tunnel Fires - Heptane pool fire case)

  • 유홍선;양승신
    • 한국터널지하공간학회 논문집
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    • 제7권2호
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    • pp.109-117
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    • 2005
  • 본 연구는 터널내 화재시 배연속도가 연소율 변화에 미치는 영향을 파악하기 위하여 Froude scaling에 의해 1/20 크기로 축소한 모형화재 실험을 수행하였다. 화원으로는 4.5cm~8.5cm의 헵탄을 사용하였으며 발열량은 3.71~15.6 kW이다. 연소율은 로드셀을 이용하여 산출하였고, 연기거동을 파악하기 위하여 K형 열전대를 이용하여 온도분포를 측정하였다. 풍동은 터널 상류 한쪽부분과 연결하였고, 터널 공간의 배연속도를 제어하기 위하여 풍동의 인버터를 조정하였다. 헵탄 풀화재인 경우 배연속도가 증가할수록 충분한 산소의 공급으로 연소율은 증가하였으며, 같은 무차원 속도($\bar{V}$) 일때 화원 크기가 작아짐에 따라 연소율은 증가하였다.

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Application of the Artificial Coral Reef as a Coastal Erosion Prevention Method with Numerical-Physical Combined Analysis (Case Study: Cheonjin-Bongpo Beach, Kangwon Province, South Korea)

  • Hong, Sunghoon;Jeong, Yeon Myeong;Kim, Taeyoon;Huynh, Van Men;Kim, Inho;Nam, Jungmin;Hur, Dong Soo;Lee, Jooyong;Kwon, Soonchul
    • 한국해양공학회지
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    • 제35권1호
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    • pp.75-81
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    • 2021
  • Artificial Coral Reefs (ACRs) have been introduced to help solve coastal erosion problems, but their feasibility has not been assessed with field data. This study conducted a feasibility analysis of ACRs on their erosion mitigation effects by performing a case study of Cheonjin-Bongpo beach, South Korea. A numerical-physical combined analysis was carried out using a SWAN model simulation and physical model test with a scale of 1/25 based on field observations of Cheonjin-Bongpo beach. Both Dean's parameter and the surf-scaling parameter were applied to comparative analysis between the absence and presence conditions of the ACR. The results for this combined method indicate that ACR attenuates the wave height significantly (59~71%). Furthermore, ACR helps decrease the mass flux (~50%), undertow (~80%), and maximum wave set up (~61%). The decreases in Dean's parameter (~66%) and the surf-scaling parameter suggest that the wave properties changed from the dissipative type to the reflective type even under high wave conditions. Consequently, an ACR can enhance shoreline stability.