Interstellar Extinction vs. Dust

Slides:

Advertisements

Similar presentations

Hydrocarbon dust in Seyfert galaxies and ULIRGs R. Mason (NOAO Gemini Science Center) G. Wright (Astronomy Technology Centre) Y. Pendleton (NASA Ames)

Advertisements

Impact of Jet Feedback on H 2 and Star Formation in Radio Galaxies Patrick Ogle (Caltech, Spitzer Science Center) R. Antonucci, C. Leipski, Phil Appleton,

REDDENING Nancy Elias de la Rosa. OUTLINE  Interstellar reddening  Extinction law – Cardelli et al.  Reddening in SNIa  Photometric methods  Spectroscopic.

Dust particles and their spectra. Review Ge/Ay 132 Final report Ivan Grudinin.

Thermonuclear Supernovae Lifan Wang Texas A&M University Oct 6, 2013.

AT20G compact HII region Survey: Spitzer character of the sources in the MIR Martin Cohen, University of California/Berkeley “Hyper Compact HII regions”

Multi-band Infrared Mapping of the Galactic Nuclear Region Q. D. Wang (PI), H. Dong, D. Calzetti (Umass), Cotera (SETI), S. Stolovy, M. Muno, J. Mauerhan,

General Astronomy The Interstellar Medium Credits: Much of this slideset is modified from lectures by Dr. Peter Newbury (UBC)

AGN Unification Viewed in the mid-IR Lei Hao Cornell University Spectra.

A new database of infrared mineral spectra for astrophysics by Anne M. Hofmeister Many thanks to Janet Bowey, Angela Speck, and Mike Barlow Star sapphire.

Polarization - Extinction Relation in the 4th Galactic Quadrant Nadia Kaltcheva Department of Physics and Astronomy, University of Wisconsin Oshkosh Statistical.

What can the Interstellar Extinction Curves Tell us About? Takaya Nozawa Masataka Fukugita (Kavli IPMU, University of Tokyo) 2012/08/07.

The nature of the dust and gas in the nucleus of NGC 1068.

CfA B.T. Draine: Dust in the submm1 Dust in the sub-mm or: what is  ? B. T. Draine Princeton University 2005 June 14.

Radio Astronomy And The Spiral Structure Of The Milky Way Jess Broderick Supervisor: Dr George Warr.

The Interstellar Medium Physical Astronomy Professor Lee Carkner Lecture 12.

The Central Engine of AGNs, XiAn, October 2006 Dust in Active Galactic Nuclei Aigen Li (University of Missouri-Columbia)

マゼラン雲中の星形成領域、分子雲中でのダストの性質

Spitzer/IRS survey of heavily obscured planetary nebula precursors planetary nebula precursors D. A. García-Hernández (McDonald Observatory, UT, USA) J.

1 Common Far-Infrared Properties of the Galactic Disk and Nearby Galaxies MNRAS 379, 974 (2007) Hiroyuki Hirashita Hiroyuki Hirashita (Univ. Tsukuba, Japan)

ASTR112 The Galaxy Lecture 10 Prof. John Hearnshaw 13. The interstellar medium: dust IRAS view of warm dust in plane of the Galaxy.

Atomic Spectroscopy for Space Applications: Galactic Evolution l M. P. Ruffoni, J. C. Pickering, G. Nave, C. Allende-Prieto.

Ia 型超新星の特異な減光則から探る系外銀河のダスト特性野沢貴也（ Takaya Nozawa ） National Astronomical Observatory of Japan 2015/06/05.

Lecture on Cosmic Dust Takaya Nozawa (IPMU, University of Tokyo) 2011/12/19 Today’s Contents: 1) Composition of dust 2) Extinction of stellar lights by.

Constraints on small grains from ISO, Spitzer data: Towards predicting the cm-emission of PAHs L. Verstraete N. FlageyIAS, Orsay M. Compiègne.

Detection of the 2175Å Dust Extinction Feature at high z Junfeng Wang (Penn State/UFL) Collaborators : Jian Ge (U. of Florida), Pat Hall (Princeton U./York.

ASTR112 Astrophysics: the Galaxy Prof. John Hearnshaw 2003 semester 1 Room 804, Rutherford Building Department of Physics and Astronomy

PX269 Galaxies Part 2: Our Galaxy, the Milky Way 2.1 Components and Structure PX269 Galaxies.

The infrared extinction law in various interstellar environments 1 Shu Wang 11, 30, 2012 Beijing Normal University mail.bnu.edu.cn.

The Differences in the SEDs of Type 1 and Type 2 AGNs: Contributions from starbursts Xue-Bing Wu Collaborator: Ran Wang (Astronomy Department, Peking University)

Stéphanie Cazaux Leon Boschman Thomas Schlathölter Ronnie Hoekstra

May 19-23Bologna pg course Evening ZL Guilleman: “The Heavens” 1896 Interstellar and interplanetary dust Michael Rowan-Robinson Imperial College.

Dust cycle through the ISM Francois Boulanger Institut d ’Astrophysique Spatiale Global cycle and interstellar processing Evidence for evolution Sub-mm.

X-shooter spectroscopy of the GRB090926A afterglow Valerio D’Elia (ASDC/INAF-OAR) & The X-shooter GRB collaboration April, 22nd Kyoto - Japan.

The Interstellar Medium. Red, White, and Blue : Nebulae.

Further studies of λ Diffuse Interstellar Band Takeshi Oka, Lew M. Hobbs, Daniel E. Welty, Donald G. York Department of Astronomy and Astrophysics,

Interstellar extinction law and its dust model in the infrared 姜碧沩北京师范大学天文系 Group members: 高健王舒李爱根 etc.

2/6/2016 DCH-1 JWST/MIRI Space Telescope Science Institute The Infrared Sky: Background Considerations for JWST Dean C. Hines & Christine Chen MIRI Instrument.

Chapter 14 The Interstellar Medium. All of the material other than stars, planets, and degenerate objects Composed of gas and dust ~1% of the mass of.

Belén Maté, Miguel Jiménez-Redondo, Isabel Tanarro, Miguel Moreno, and Victor Herrero Instituto de Estructura de la Materia (IEM-CSIC), Serrano 123, 28006,

Chap 3 – Interstellar Dust. Problem We have no direct probes / samples of true interstellar dust. Everything we know comes from its interaction with light:

Galactic Extinction Curves and Interstellar Dust Models Nozawa, T. and Fukugita, M. (Kavli IPMU, University of Tokyo) 2012/05/08.

Radiation fields in the Milky Way and their role in High-Energy Astrophysics Richard Tuffs, Ruizhi Yang, & Felix Aharonian (MPI-Kernphysik Heidelberg)

Cosmic Dust Enrichment and Dust Properties Investigated by ALMA Hiroyuki Hirashita ( 平下博之 ) (ASIAA, Taiwan)

Variation of the 9.7 µm Silicate Absorption Feature with Extinction in the Dense Interstellar Medium Megan M. Bagley with Dr. Jean E. Chiar, SETI Institute.

IR Spectroscopy. 6. Interstellar Medium  Hot ISM : hot ionized matter at very low density ( n ~ 5x10 -3 cm -3 ) and heated to very high temperature (~

“SPITZER observations of luminous obscured Quasars” Enrica Bellocchi in collaboration with A. Comastri, F. Pozzi, C. Vignali, J. Fritz, L. Pozzetti on.

減光曲線から探る星間ダストの多様性 ( Variation of interstellar dust probed by extinction curves) 野沢貴也 (Takaya Nozawa) & 福来正孝 (Masataka Fukugita) (Kavli IPMU, University.

Astromineralogy of Protoplanetary Disks (and other astrophysical objects) Steve Desch Melissa Morris Arizona State University.

Peter Sarre Alessandra Candian, Markus Hammonds, Tom Kerr,

Infrared Polarization and Interstellar Grain Models 红外偏振与星际尘埃模型李祺（湘潭大学）导师：李爱根星际尘埃模型：简介星际偏振对尘埃模型的限止结果与讨论 2014年7月15－19日大连.

On the reddening law observed for Type Ia Supernovae

The Near-Infrared Extinction Laws and Distance Estimation of Monoceros Nebula He Zhao Biwei Jiang

Mid- Infrared Spectroscopic Properties of IR QSOs

星际物理与化学（大连）讨论会 Dust in the Local Group, AGNs, and High-z Universe Aigen Li (University of Missouri) 16 - July

Part 2: The Milky Way 2.1 Components and Structure

Dust extinction, emission & polarisation in the diffuse ISM

Thomas D. Varberg, Department of Chemistry, Macalester College, St

Infrared Universe to be seen by QDs

Galactic Astronomy 銀河物理学特論 I Lecture 1-6: Multi-wavelength properties of galaxies Seminar: Draine et al. 2007, ApJ, 663, 866 Lecture: 2011/11/14.

2014/09/13 高赤方偏移クェーサー母銀河の星間ダスト進化と減光曲線 (Evolution of interstellar dust and extinction curve in the host galaxies of high-z quasars) 野沢貴也（Takaya Nozawa）

Dust Models for the Extinction of Type IIn SN 2010jl Jian Gao, Jun Li, B. W. Jiang Beijing Normal University , 昆明.

(National Astronomical Observatory of Japan)

by Th. Henning, and F. Salama

2010/12/16 Properties of interstellar and circumstellar dust as probed by mid-IR spectroscopy of supernova remnants (超新星残骸の中間赤外分光から探る星間・星周ダスト) Takaya.

2016/09/16 Properties of Interstellar Dust as Probed by Extinction Laws toward Type Ia Supernovae Takaya Nozawa (National Astronomical Observatory of Japan)

Peculiar Extinction Laws observed for Type Ia Supernovae

Ia型超新星の特異な減光則を引き起こす母銀河ダストの性質

2017/01/23 Properties of Dust Accounting for Extinction Laws toward Type Ia Supernovae (Nozawa, T. 2016, Planetary and Space Science, 133, 36) Takaya Nozawa.

Dust Polarization in Galactic Clouds with PICO

Presentation transcript:

Interstellar Extinction vs. Dust 姜碧沩 Department of Astronomy Beijing Normal University

2015/7/13 星际/星周尘埃 2015 暑期班

2015/7/13 星际/星周尘埃 2015 暑期班

2015/7/13 星际/星周尘埃 2015 暑期班

Principal features General rise from IR to UV (~0.1μm) 18μm and 10μm: O-Si-O bend and Si-O stretch in amorphous silicate 3.4μm: C-H stretch in hydrocarbon 2175Å: “2200 bump”. Probably pi – pi* electronic transition in sp2-bonded carbon (e.g. graphite or PAH) 400+ weak features – the Diffuse Interstellar Bands – still unidentified 2015/7/13 星际/星周尘埃 2015 暑期班

红外消光的强度红外测光的精度消光改正的难度红外的深度 Galactic Center Gao, Li, Jiang, 2013 EPS, 65,1127 2015/7/13 星际/星周尘埃 2015 暑期班

Inhomogeneity of Interstellar Extinction Extinction law 2D extinction 3D extinction 2015/7/13 星际/星周尘埃 2015 暑期班

2015/7/13 星际/星周尘埃 2015 暑期班 Draine 2003 ARAA

Schelgel et al. 1998 2015/7/13 星际/星周尘埃 2015 暑期班

Chen, Schultheis, Jiang et al 2013 2015/7/13 星际/星周尘埃 2015 暑期班

Determination of Extinction Color excess Intrinsic color index stars Line ratio Nebula Pair-method Spectrum 2015/7/13 星际/星周尘埃 2015 暑期班

vs. Dust 2015/7/13 星际/星周尘埃 2015 暑期班

2015/7/13 星际/星周尘埃 2015 暑期班

CCM89 2015/7/13 星际/星周尘埃 2015 暑期班

2015/7/13 星际/星周尘埃 2015 暑期班

FM90 UV extinction curve 2015/7/13 星际/星周尘埃 2015 暑期班

Wang et al. 2013 2015/7/13 星际/星周尘埃 2015 暑期班

Summary Dust produces extinction, extinction reveals dust 2015/7/13 星际/星周尘埃 2015 暑期班 Trumpler, R. 1930 PASP 42, 21

Influence of Extinction Herschel's Map of the Milky Way On the Construction of the Heavens. By William Herschel, Esq. F. R. S. Philosophical Transactions of the Royal Society of London, Vol. 75. (1785), pp. 213-266. 2015/7/13 星际/星周尘埃 2015 暑期班