'Dust mass' presentation slideshows

On Dust in the Early Universe

On Dust in the Early Universe. Takaya Nozawa (IPMU, University of Tokyo). Contents: 1. Observations of dust at high-z 2. Formation of dust in supernovae 3. Critical metallicity 4. EMP-stars and dust. 2010/07/29. 1. Observations of dust at high-z.

585 views • 45 slides

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2018/10/15. ???????????? ????? SiC ????? (Issues of dust formation in supernovae and Formation of SiC grains in supernovae). ?? ?? ? Takaya Nozawa ? ????? ????? (Division of theoretical astronomy, NAOJ). Special thanks: Masaomi Tanaka (Tohoku Univ.) ,

354 views • 35 slides

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2012/09/05. ???????????????????????????. ?????? Takaya Nozawa ? ???? ??????? ?????????????? Kavli I PMU ?. Collaborators; T. Kozasa , A. Habe (Hokkaido University) K. Maeda , K. Nomoto (IPMU), H. Umeda (U.T.) N. Tominaga (Konan Univ.). 1. Introduction.

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Dust and PAHs in X-ray Plasma of Elliptical Galaxies Hidehiro Kaneda ? Nagoya U. ? , et al.

Dust and PAHs in X-ray Plasma of Elliptical Galaxies Hidehiro Kaneda ? Nagoya U. ? , et al. Ellipticals: ? old stars not productive of dust ? hot plasma destructive to dust BUT, dust still exists despite harsh environments. X-ray. visible. IR. AKARI 3 m m. d = 1 arcmin.

412 views • 26 slides

Supernovae as sources of interstellar dust

Supernovae as sources of interstellar dust. Takaya Nozawa (IPMU, University of Tokyo). Thanks to: T. Kozasa (Hokkaido Univ.), N. Tominaga (Konan Univ.) K. Maeda , M. Tanaka , K. Nomoto (IPMU, Univ. of Tokyo) H. Umeda , I. Sakon (University of Tokyo). 2011/06/21. Outline.

382 views • 25 slides

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2014/05/07. ?????????? ???????????. ?? ??? Takaya Nozawa ? (National Astronomical Observatory of Japan ). Main collaborators: T. Kozasa , A. Habe (Hokkaido University) H. Umeda (University of Tokyo) K. Maeda (Kyoto University), K. Nomoto ( Kavli IPMU)

364 views • 25 slides

385 views • 24 slides

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2014/04/21. ??????????????? ?????. ?? ??? Takaya Nozawa ? (National Astronomical Observatory of Japan ). Main collaborators: T. Kozasa , A. Habe (Hokkaido University) K. Maeda (Kyoto University), K. Nomoto ( Kavli IPMU) H. Umeda (University of Tokyo) , M. Tanaka (NAOJ)

326 views • 24 slides

Probing Dust Formation Process in SN 1987A with ALMA

2013/10/22. Probing Dust Formation Process in SN 1987A with ALMA. Takaya Nozawa (Kavli IPMU) and Masaomi Tanaka (NAOJ). 1-1. Introduction. SNe are important sources of interstellar dust? ? huge amounts of dust grains (>10 8 M sun ) are detected

352 views • 23 slides

Detecting Cool Dust in SNRs in LMC and SMC with ALMA

Detecting Cool Dust in SNRs in LMC and SMC with ALMA. Takaya Nozawa (Kavli IPMU) and Masaomi Tanaka (NAOJ). Targets ? SN 1987A: our proposal for ALMA Cycle 0 and next plan for ALMA Cycle 1 ? 1E0102.2-7219: youngest SNR in SMC. 2012/6/11.

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Early results from the IRS

Early results from the IRS. Jim Houck and the IRS team - AAS Denver 6/1/04. IRS Status. The hardware is working well: The responsively is better than expected The noise is the same as in the lab Suffered a major solar proton event; 2.5 year dose in 2.5 days!

267 views • 15 slides

Mid-infrared Observations of Aged Dusty Supernovae

2013/05/24. Mid-infrared Observations of Aged Dusty Supernovae. Takaya Nozawa ??? ??? (Kavli I PMU, University of Tokyo). special thanks: Tanaka, M., Arimatsu , K., Ohsawa , R., Sakon , I. 1-1. Origin of IR emission from SNe. Dust formation in the ejecta.

231 views • 15 slides

Shinya Komugi NAOJ Chile Observatory + Rie Miura, Sachiko Onodera, Tomoka Tosaki, Nario Kuno

MAGiC IV : ?????????. Shinya Komugi NAOJ Chile Observatory + Rie Miura, Sachiko Onodera, Tomoka Tosaki, Nario Kuno + many (NRO Legacy MAGiC team, ASTE team, AzTEC team). NRO UM Jul. 25 2013. Star formation relation within M33. Increased scatter at 100pc scale Effect of GMC evolution ?

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Dust in edge-on spiral galaxies from the J-band of the 2MASS Large Galaxy Atlas

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Dust emission in SNR 1987A and high-z dust observations

2013/10/24. Dust emission in SNR 1987A and high-z dust observations. Takaya Nozawa (Kavli IPMU). ? Contents of this talk - Introduction - Our ALMA proposals for SNR 1987A - Infrared Emission of Dust Grains - Extinction Curves in high-z Galaxies - Summary.

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Revealing the mass of dust formed in the ejecta of SNe with ALMA ALMA ???????????????????

Revealing the mass of dust formed in the ejecta of SNe with ALMA ALMA ???????????????????. Takaya Nozawa (IPMU, University of Tokyo). Collaborators; M. Tanaka (IPMU), I. Sakon (University of Tokyo), T. Kozasa, T. Minamidani (Hokkaido University),

269 views • 12 slides

Massive-Star Supernovae as Major Dust Factories

Massive-Star Supernovae as Major Dust Factories.

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Detecting the signature of planets at millimeter wavelengths

Francisco Ramos Stierle : David Hughes : Edward Chapin :. framos@inaoep.mx dhughes@inaoep.mx echapin@inaoep.mx. Detecting the signature of planets at millimeter wavelengths. F. Ramos-Stierle, D.H. Hughes, E. L. Chapin (INAOE, Mexico ), G.A. Blake ??? gab@gps.caltech.edu.

108 views • 1 slides

Detecting the signature of planets at millimeter wavelengths

Francisco Ramos Stierle : David Hughes : Edward Chapin :. framos@inaoep.mx dhughes@inaoep.mx echapin@inaoep.mx. Detecting the signature of planets at millimeter wavelengths. F. Ramos-Stierle, D.H. Hughes, E. L. Chapin (INAOE, Mexico ), G.A. Blake ??? gab@gps.caltech.edu.

88 views • 1 slides