Mid-Infrared Observations of Planet Forming Material Orbiting Young Stars Eric Leibensperger Ithaca College.

Slides:



Advertisements
Similar presentations
Probing the Conditions for Planet Formation in Inner Protoplanetary Disks James Muzerolle.
Advertisements

Spitzer IRS Spectroscopy of IRAS-Discovered Debris Disks Christine H. Chen (NOAO) IRS Disks Team astro-ph/
Extended IR Emission from LIRGs V. Charmandaris, T. Diaz-Santos, (Univ. of Crete) L. Armus & A. Petric (SSC/Caltech)
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,
Dust particles and their spectra. Review Ge/Ay 132 Final report Ivan Grudinin.
Physical Properties of Spectroscopically-Confirmed z>6 Galaxies By Charles Griffin With special thanks to Dr. Eiichi Egami, and Dr. Benjamin Clément NASA.
Elisabete da Cunha (ESR – IAP) MAGPOP Mid Term Review – La Palma, MAGPOP ESR at the Institut d’Astrophysique de Paris MAGPOP Mid Term Review La.
Detecting the signature of planets at millimeter wavelengths F. Ramos-Stierle, D.H. Hughes, E. L. Chapin (INAOE, Mexico ), G.A. Blake ???
Hot Molecular Gas Orbiting Young Stars: Planet Forming Disks or Small Stellar Companions? A look at data taken at the 200” Mount Palomar Telescope, and.
Star Formation with PILOT: Science in the thermal infrared Michael Burton University of New South Wales.
Discovery of an Extraordinarily Massive Young Stellar Cluster Donald F. Figer Rochester Institute of Technology/STScI J. MacKenty, M. Robberto, K. Smith.
Research in Astronomy: Studying Big Stars, Small Stars, And Working with Computers (a.k.a. the cool stuff I’ve done since last January)
TIGER The TIGER Instrument Overview Phil Hinz - PI July 13, 2010.
Study of Planet forming Systems Orbiting Intermediate-mass Stars Sweta Shah Ithaca College Advisor: Dr. Luke Keller In collaboration with the NASA Spitzer.
Scientists Find Possible Birth of Tiniest Known Solar System ? Jeng-Lwen, Chiu Institute of Physics, NTHU 2005 / 12 / 15.
Pre-Main Sequence Stars PHYS390 (Astrophysics) Professor Lee Carkner Lecture 13.
Infrared Identification of Forming Solar Systems in Other Galaxies Sweta Shah Ithaca College Advisor: Dr. Luke Keller Physics Department Small Magellanic.
Comparison of Photometric And Spectroscopic Redshifts.
Mid-IR High Ionization Lines in Starbursts Lei Hao Spitzer IRS Team Cornell University.
Centimeter and Millimeter Observations of Very Young Binary and Multiple Systems -Orbital Motions and Mass Determination -Truncated Protoplanetary Disks.
Lecture 16: Searching for Habitable Planets: Remote Sensing Methods and parameters we can measure Mean density measurements: internal structure Measurements.
Black Hole in M83 Topic: Black holes Concepts: multi-wavelength observations, black hole evolution Missions: Hubble, Chandra, Swift Coordinated by the.
Margaret Meixner (STScI, JHU) March 7, 2013
Infrared Telescopes 1.
The Galactic Centre: a hidden treasure How can we study the Galactic centre? How can we study the Galactic centre? What is do we find there? What is do.
2005 June 2260th Symposium on Molecular Spectroscopy Outflows and Magnetic Fields in L1448 IRS3 Woojin Kwon Leslie W. Looney Richard M. Crutcher Jason.
Astrophysics from Space Lecture 8: Dusty starburst galaxies Prof. Dr. M. Baes (UGent) Prof. Dr. C. Waelkens (KUL) Academic year
9. Distances in open space China Zhu. Statement of problem 9 How do astronomers measure distances between the planets of the Solar System, between the.
Stars are born from a large collection of dusts and gasses that compress under the pressure of gravity, and eventually these dusts and gasses clump in.
L. Matrà 1,2, B. Merín 1, C. Alves de Oliveira 1, N. Huélamo 3, Á. Kóspál 4, N. L.J. Cox 5, Á. Ribas 1,3, E. Puga 1, R. Vavrek 1, P. Royer 5, T. Prusti.
1 BDRv3 - November 26, Markus Kissler-Patig E-ELT Programme 1 E-ELT Science Case Markus Kissler-Patig.
Ralf Siebenmorgen MIR on ELT’s The Mid-infrared on ELT’s MIR recommended to be essential (3 – 25µm)
Protoplanetary discs of isolated VLMOs discovered in the IPHAS survey Luisa Valdivielso (IAC) ‏ Collaborators: E. Martín, H. Bouy, E. Solano, J.Drew, R.
Lecture 14: The Discovery of the World of Exoplanets Indirect methods for planet detection The Astrometric method The Doppler shift method The Transit.
Spitzer IRS spectra of PAH emission from
Universities Space Research Association Page 1 Communications Integrated Systems FLITECAM – Compelling Science Ian McLean UCLA.
Schematic Picture of Region close to protostar From Matt & Pudritz (2005) disk envelope outflow.
Image Processing: Critical to Hubble Discoveries
Hubble Space Telescope Mrs. Ott Example. History Orbits 370 miles above Earth Building began in 1977 by NASA Named after scientist Edwin Hubble Placed.
Thessaloniki, Oct 3rd 2009 Cool dusty galaxies: the impact of the Herschel mission Michael Rowan-Robinson Imperial College London.
EMBARGOED UNTIL 22 JULY 2010 Detection of C60 and C70 in a Young Planetary Nebula Jan Cami,1,2* Jeronimo Bernard-Salas,3,4 Els Peeters,1,2 Sarah Elizabeth.
Searching for extra-solar planets in Infrared J. Serena Kim Steward Observatory, Univ. of Arizona In collaboration with FEPS Spitzer legacy team (
Other planetary systems Are there other “solar systems” out there?
Young Star Disk Evolution in the Planet Formation Epoch Gregory Mace Mentor: Lisa Prato Northern Arizona University Physics and Astronomy.
PI Total time #CoIs, team Silvia Leurini 24h (ALMA, extended and compact configurations, APEX?) Menten, Schilke, Stanke, Wyrowski Disk dynamics in very.
NIR, MIR, & FIR.  Near-infrared observations have been made from ground based observatories since the 1960's  Mid and far-infrared observations can.
Instrument, Data Reduction, and Preliminary Results DU Graduate Student Colloquium Kathy Geise Image Courtesy NASA/JPL-Caltech.
Why is water interesting? Evidence of water in space Water in young disks Water in the terrestrial planet-forming zone Future prospects Water in young.
Spitzer Space Telescope Mww-1 Warm Spitzer and Astrobiology Presented to NASA Astrobiology Institute Planetary System Formation Focus Group Michael Werner.
Telescope Technology Types of Telescopes Hubble Telescope and NASA’s Great Observatories.
Circumstellar Disks at 5-20 Myr: Observations of the Sco-Cen OB Association Marty Bitner.
Peter Sarre Alessandra Candian, Markus Hammonds, Tom Kerr,
A New Approach to Galaxy Formation— The Universe Going Green
The Science of Creation
The Interstellar Medium and Star Formation
Herschel Space Observatory
Observing and Data Reduction
The Interstellar Medium and Star Formation
The Science of Creation
W3 Preliminary Polarimetry Data
NASA discovery (22th February 2017):
Observing Planets and Stars
Polarizing Coronagraph for Circumstellar Dust Observations
A Study of Accretion Disks Around Young Binary Star Systems
Dynamical Mass Ratios of the Youngest Low-Mass Stars
-Orbital Motions and Mass Determination
The Search for Planet Forming Regions in Young Binaries
Observational Tools of Space Rubric
Evolution of Gas in Circumstellar Disks
Presentation transcript:

Mid-Infrared Observations of Planet Forming Material Orbiting Young Stars Eric Leibensperger Ithaca College

Overview ● Star and Planet Formation ● Observations and Data Reduction ● Results ● Conclusions and Future Work

Star and Planet Formation

Observations and Data Reduction ● Spitzer Space Telescope Infrared Spectrograph (IRS) ● ~ 300 of 600 stars have been observed ● Reduction with SMART (Spectroscopy Modeling Analysis and Reduction Tool) Wavelength Intensity SMART Extraction (2 dimensional to 1 dimensional)

Results

Results cont. Disk Orientation

Conclusions and Future Work ● Standardized procedure to reduce data ● Strong evidence for circumstellar disks of planet forming material ● Orientation of disk can be determined ● Discovery of young star with cleared inner disk which implies planet formation ● Future Work: Detailed study of polycyclic aromatic hydrocarbon emission in Herbig Ae/Be (massive young) stars Wavelength ( μm) Intensity (Jy) PAH Emission from a young star