Diffuse Interstellar Bands: HD

Slides:

Advertisements

Similar presentations

A Search for C 4 and C 5 in the (Molecular) Carbon-Rich Sightline toward HD Máté Ádámkovics (UC Berkeley), Geoffrey A. Blake (Caltech), Ben McCall.

Advertisements

Infrared Space Astrometry mission for the Galactic Bulge

SN1014J in M82 A Pseudo-GOTOQ and what we can learn with really big telescopes and DIBs about QSOALS Donald G. York, Dan Welty, Jiaqi Jiang University.

APO and Diffuse Interstellar Bands Donald G. York University of Chicago APO 20 th (30 th ?) reunion May 12, 2014.

Implications of the H H 2  H 2 + H 3 + reaction for the ortho- to para-H 3 + ratio in interstellar clouds Kyle N. Crabtree, Lt. Col. Brian A. Tom,

Finding the First Cosmic Explosions Daniel Whalen McWilliams Fellow Carnegie Mellon University.

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

ASTRONOMICAL APPLICATIONS OF NEW LINE LISTS FOR CN, C 2 AND THEIR ISOTOPOLOGUES P. F. Bernath Department of Chemistry and Biochemistry, Old Dominion University,

Benjamin McCall and Takeshi Oka University of Chicago Kenneth H. Hinkle National Optical Astronomy Observatories Thomas R. Geballe Joint Astronomy Centre.

The Non-Thermal Rotational Distribution of Interstellar H 3 + (ApJ, in press ) Takeshi Oka and Erik Epp, Department of Astronomy and Astrophysics, and.

Galactic Center Region Concentrated stars and interstellar matter High Energy Density (gravity, MHD, kinetic) Strong magnetic field :B ~ mG High external.

1 Non-linear Effects of Atmospheric Extinction on Observations in Astronomy Frédéric Zagury Institut Louis de Broglie Paris - France.

Hot and Diffuse Gas near the Galactic Center Probed by Metastable H 3 + Thomas R. Geballe Gemini Observatory Miwa Goto Max Planck Institute for Astronomy.

Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center from 140 pc West to 85 pc East of Sgr A* 66th OSU International Symposium, June.

The Galactic center region Concentrated stars and interstellar matter High energy density (gravity, MHD, kinetic) Strong magnetic field :B ~ mG High external.

CH +, CH, and CN Emission from the Red Rectangle Lewis M. Hobbs, Julie A. Thorburn, D. G. York, Takeshi Oka, Department of Astronomy and Astrophysics,

H3+H3+. H 3 +, a new astrophysical probe: Revelation of warm and diffuse gas near the Galactic center Takeshi Oka Department of Astronomy and Astrophysics.

HD , the C 2, C 3 rich sightline. The C 2 Diffuse Interstellar Bands Takeshi Oka Department of Astronomy and Astrophysics And Department of Chemistry.

Pedro GARCIA-LARIOPlanetary Nebulae as Astronomical Tools / Gdańsk, June 28/July , Page 1 o The use of PNe precursors in the study of Diffuse Interstellar.

Space Physics and Astronomy Dr. Darrel Smith, Chair Department of Physics College of Arts & Sciences Temasek Polytechnic Visit September 6, 2013.

Absorption line survey toward the Galactic center II Miwa Goto Max-Planck-Institut fuer Astronomie Heidelberg, Germany contribution from Subaru to the.

$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.

On the discovery of the diffuse interstellar bands by Benjamin J. McCall, and R. Elizabeth Griffin Proceedings A Volume 469(2151): March 8, 2013.

Brian Siller, Andrew Mills, Michael Porambo & Benjamin McCall University of Illinois at Urbana-Champaign.

$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.

Modeling Linear Molecules as Carriers of the 5797 and 6614 Å Diffuse Interstellar Bands Jane Huang, Takeshi Oka 69 th International Symposium on Molecular.

Lineshape and Sensitivity of Spectroscopic Signals of N 2 + in a Positive Column Collected Using NICE-OHVMS Michael Porambo, Andrew Mills, Brian Siller,

赴国际水稻所访学情况汇报长江大学农学院邢丹英 2010 年 6 月. 学习目的学习时间、地点学习内容学习收获几点体会汇报提纲.

Lineshape and Sensitivity of Spectroscopic Signals of N 2 + in a Positive Column Collected Using NICE-OHVMS Michael Porambo, Andrew Mills, Brian Siller,

Spectroscopy of H 3 + and CO toward the Galactic center Takeshi Oka, Christopher P. Morong, Department of Astronomy And Astrophysics and Department of.

The Nearly Perfect Correlation between the Diffuse Interstellar Bands λλ and Ben McCall Department of Chemistry and Department of Astronomy.

Molecular Interstellar Absorption toward the Pleiades Star Cluster Adam Ritchey Department of Physics & Astronomy University of Toledo June 21, 2006.

November 6, 2010 MWAM 2010 University of Illinois1 The ortho:para ratio of H 3 + in diffuse molecular clouds Kyle N. Crabtree, Nick Indriolo, Holger Kreckel,

FC10; June 25, 2010Image credit: Gerhard Bachmayer Constraining the Flux of Low- Energy Cosmic Rays Accelerated by the Supernova Remnant IC 443 N. Indriolo.

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

The anomalous DIBs in the spectrum of Herschel 36 II. Analysis of radiatively excited CH +, CH, and diffuse interstellar bands Takeshi Oka, Daniel E. Welty,

The anomalous DIBs in the spectrum of Herschel 36 II. Analysis of radiatively excited CH +, CH, and diffuse interstellar bands Takeshi Oka, Daniel E. Welty,

Fourier Transform Emission Spectroscopy of the B 2 Σ + -X 2 Σ + (Violet) System of CN R.S. Ram Department of Chemistry, University of Arizona, Tucson,

Analysis of Anomalous DIBs in the Spectrum of Herschel 36 Takeshi Oka, Daniel E. Welty, Sean Johnson, Donald G. York, Julie Dahlstrom, and Lew Hobbs Department.

Tyler P. Troy, Scott H. Kable, Timothy W. Schmidt Department of Chemistry, University of Sydney Scott A. Reid Department of Chemistry, Marquette University.

Diffuse Interstellar Bands, Atoms, and Small Molecules

Central Molecular Zone (CMZ): the Treasure House of H 3 + Takeshi Oka Thomas R. Geballe Gemini Observatory Miwa Goto Max Planck Institute for Astronomy.

Searching for Vibronic Progressions in the Diffuse Interstellar Bands via Agglomerative Clustering Jane Huang Astro 193 Final Project Spring 2015.

南水北调东线第一期工程山东段情况简介. 主要汇报内容二、南水北调山东段工程总体布置三、山东段工程项目划分及工程主要建设内容一、南水北调东线工程概况四、前期工作及工程建设进展情况五、工程总投资.

June 19, 2008University of Illinois at Urbana-Champaign 1 Constraining the Low-Energy Cosmic Ray Spectrum Nick Indriolo, Brian D. Fields, Benjamin J. McCall.

(Figure provided by Adolf Witt) MBM12 Interstellar Cloud Studied 13 stars around Made of dust and gas ~100x50 pc.

The Enigmatic Diffuse Interstellar Bands: A Reservoir of Organic Material Ben McCall Department of Chemistry and Department of Astronomy University of.

Dave Meyer Northwestern University Optical/UV Absorption Line Observations of Small-Scale Interstellar Structure.

The Performance Of A Continuous Supersonic Expansion Discharge Source

The Performance Of A Continuous Supersonic Expansion Discharge Source

Radioactive elements in metal deficient stars

Nuclear Spin Dependence of the Reaction of H3+ with H2

Nature and spectral variation of B-type emission-line stars with compact dusty envelopes: HD 85567 and AS 386 Khokhlov Serik.

A Green Bank Telescope Search for ortho-benzyne (o-C6H4) in CRL 618

COUNTING IN BINARY Binary weightings 0 x x x x 8

CH+ spectrum and diffuse interstellar bands

Mitsunori ARAKI, Hiromichi WAKO, Kei NIWAYAMA and Koichi TSUKIYAMA○

arXiv: OBSERVATIONS AND ANALYSIS

Nick Indriolo1, Thomas R. Geballe2, Takeshi Oka3, and Benjamin J

Tokyo Univ. Science Mitsunori Araki, Yuki Matsushita, Koichi Tsukiyama

Can We Use Metastable Helium to Trace the Cosmic-Ray Ionization Rate?

Probing Cosmic-Ray Acceleration and Propagation with H3+ Observations

Observation of H3+ in the Diffuse Interstellar Medium

Can We Use Metastable Helium to Trace the Cosmic-Ray Ionization Rate?

Investigating the Cosmic-Ray Ionization Rate in the Galactic Interstellar Medium through Observations of H3+ Nick Indriolo,1 Ben McCall,1 Tom Geballe,2.

A New Catalog of Diffuse Interstellar Bands

International Symposium on Molecular Spectroscopy

Lab 9 – Ages and Distances to Clusters

Nuclear spin of H3+ in diffuse molecular clouds

Presentation transcript:

Diffuse Interstellar Bands: HD 183143 A New Atlas of the Diffuse Interstellar Bands: HD 183143 Lewis M. Hobbs Yerkes, U. Chicago Donald G. York U. Chicago Julie A. Thorburn Dahlstrom Carthage College Theodore P. Snow U. Colorado Michael Bishof U. Chicago Scott D. Friedman STScI Benjamin J. McCall U. Illinois Takeshi Oka U. Chicago Brian Rachford Embry-Riddle Paule Sonnentrucker STScI Daniel E. Welty U. Illinois

The APO DIB Survey Apache Point Observatory 3.5-meter 3,600–10,200 Å ; / ~ 37,500 (8 km/s) 119 nights, from Jan 1999 to Jan 2003 S/N (@ 5780Å) > 500 for 160 stars (114 reddened) Measurements & analysis still very much underway

Our Previous Atlas: HD 204827 EB-V=1.11, V=7.94 Strongest “C2 DIBs” Highest column density of C3 Double-lined spectroscopic binary! Spectral Types O9.5 V & B0.5 III 380 DIBs unambiguously detected ApJ 680, 1256 (2008) HD 204827 Credit: robgendlerastropics.com

Our Newest Atlas: HD 183143 EB-V= 1.27, V=6.92, B7Iae [Unfortunately, not a binary!] Well studied by Herbig, others No detectable C2 or C3 Distinct chemical environment 414 DIBs detected (135 are “new”) DIB population systematically redder, broader, and stronger than HD 204827 Total DIB count now ~545

Our Website: http://dibdata.org

http://dibdata.org