astronomy brown bag seminar time series analysis of hr 1040 september 16, 2008 david corliss

20
ASTRONOMY BROWN BAG SEMINAR ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS TIME SERIES ANALYSIS OF HR 1040 OF HR 1040 SEPTEMBER 16, 2008 SEPTEMBER 16, 2008 DAVID CORLISS DAVID CORLISS www.wikisky.org

Upload: brad

Post on 08-Jan-2016

20 views

Category:

Documents


0 download

DESCRIPTION

ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS. www.wikisky.org. ROCKET SCIENCE. OUTLINE. HR 1040. OBSERVATIONAL METHODOLOGY. CHALLENGES. www.wikisky.org. TIME SERIES STUDY. FUTURE RESEARCH. HR 1040 – Basic Data. Class: A0 Ia - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

ASTRONOMY BROWN BAG SEMINARASTRONOMY BROWN BAG SEMINAR

TIME SERIES ANALYSISTIME SERIES ANALYSISOF HR 1040OF HR 1040

SEPTEMBER 16, 2008SEPTEMBER 16, 2008

DAVID CORLISSDAVID CORLISS www.wikisky.org

Page 2: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

OUTLINEOUTLINE

HR 1040HR 1040OBSERVATIONAOBSERVATIONA

L L METHODOLOGYMETHODOLOGY

CHALLENGESCHALLENGESTIME SERIES TIME SERIES STUDYSTUDY

FUTURE RESEARCHFUTURE RESEARCH

ROCKET

SCIENCE

www.wikisky.org

Page 3: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

Class: A0 Ia

Distance: 758 ± 250 pc

mv: 4.54, Mv: -7.1 (Variable ± 0.3)

Teff: 9730 ± 300 K

Mass: 19.3 ± 3.3 Mּס

Radius: 97 ± 2.4 Rּס

Terminal Velocity: 218 ± 44 kms-1

Escape Velocity: 233 ± 47 kms-1

Mass Loss: 8.5 ± 3 x 10-8 Mּס yr-1

Features: Irregular Variable, Mass Loss, HVA Events

HR 1040 – Basic Data

www.wikisky.org

Page 4: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

HR 1040 – CAM OB1 ASSOCIATION

Straizys, V. & Laugalys, V., 2007, Baltic Astronomy, 16, 167

Page 5: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

OBSERVATIONS: METHODOLOGYOBSERVATIONS: METHODOLOGY

RITTER OBSERVATORY

1.06 m, f/8 Ritchey – Chrétien Telescope

High-Resolution Échelle Spectrograph

CCD Camera (Prior to 2007)1200 x 800 pixels 22.5 x 22.5 μm

cooled to 140 K

Resolution ~ 26,000 near Hα

Page 6: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

A Digital Spectral Classification Atlas, R. O. Gray, ASU

OBSERVATIONS: SPECTRUMOBSERVATIONS: SPECTRUM

Page 7: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

OBSERVATIONS: HOBSERVATIONS: Hαα PROFILE PROFILEP Cygni Mass Loss P Cygni Mass Loss

Hα Region of P Cygni, N. Richardson, M.S. Thesis, 2006

Page 8: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

OBSERVATIONS: OBSERVATIONS: HHαα Profile in HR Profile in HR 10401040

Hα Region of HR 1040, N. D. Morrison, 1993

Page 9: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

OBSERVATIONS: OBSERVATIONS: High Velocity Absorption in HR High Velocity Absorption in HR

10401040

C. L. Mulliss, 1993

Page 10: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

OBSERVATIONS: OBSERVATIONS: High Velocity Absorption in HR High Velocity Absorption in HR

10401040

N. D. Morrison, 1993

Page 11: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

CHALLENGES

Telluric Water Vapor

Hα Region of Deneb, N. Richardson, M.S. Thesis, 2006

Page 12: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

CHALLENGESSparse and intermittent data

Northern Declination - Observations can be limited

REALLY! I STUDY HR

1040

I STUDYΒ ORIONIS

Complex Hα Profile

Large Distance Contributes to Uncertainties

Page 13: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

TIME SERIES ANALYSIS:TIME SERIES ANALYSIS:

PERIODICITY PERIODICITY

Strömgren Photometry of Deneb in Fall 1999, N. Richardson, M.S. Thesis, 2006

Page 14: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

TIME SERIES ANALYSIS:TIME SERIES ANALYSIS:

FORECASTINGFORECASTING

Page 15: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

TIME SERIES ANALYSIS:TIME SERIES ANALYSIS:CHAOS CHAOS

When change makes all the When change makes all the difference!difference!

U.S. AVERAGE - REGULAR GAS

1.82.02.2

2.42.62.83.03.2

3.43.63.8

Oct 10,2006

Jan 18,2007

Apr 28,2007

Aug 06,2007

Nov 14,2007

Feb 22,2008

Jun 01,2008

Page 16: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

TIME SERIES ANALYSIS:TIME SERIES ANALYSIS:

ARIMA MODELSARIMA MODELS

1,1,0 ARIMA 1,1,0 ARIMA MODELMODEL

SMOOTH DATASMOOTH DATA

0,1,1 ARIMA 0,1,1 ARIMA MODELMODEL

CHAOTIC DATACHAOTIC DATA

METRO DETROIT TESTSCORES VS INCOME

0

20

40

60

80

100

0 10 20 30 40 50

INCOME PER CAPITA ($1,000)

M.E

.A.P

. PAS

S / F

AIL

%

U.S. AVERAGE - REGULAR GAS

1.82.02.2

2.42.62.83.03.2

3.43.63.8

Oct 10,2006

Jan 18,2007

Apr 28,2007

Aug 06,2007

Nov 14,2007

Feb 22,2008

Jun 01,2008

Page 17: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

TIME SERIES ANALYSIS:TIME SERIES ANALYSIS:

CHANGES IN CHEMISTRYCHANGES IN CHEMISTRY

Hα Region of Deneb, N. Richardson, M.S. Thesis, 2006

Page 18: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

Opportunities for further research include:

FUTURE RESEARCH

Longer Time Series

New Objects

New mathematical Techniques

Chemical Composition

Page 19: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

High Velocity Absorption events are observed and appear to be associated with variations in luminosity

CONCLUSIONS

HR 1040 is an A0 Ia Supergiant Variable

HVA events may be periodic but this can not be verified with the data presently available – more observations over longer time periods are needed

P Cygni Hα profile indicates the presence of mass loss; Rate of loss is 8.5 ± 3 x 10-8 Mּס yr-1

Standard statistical techniques for Time Series Analysis such as ARIMA Models may be useful in understanding the behavior of HR 1040

Page 20: ASTRONOMY BROWN BAG SEMINAR TIME SERIES ANALYSIS OF HR 1040 SEPTEMBER 16, 2008 DAVID CORLISS

Bright Star Catalog, Fifth Edition, 1991 (19950214)

Corliss, D. J., 2008, UT Graduate Research Symposium

Fischer, W. J. & Morrison, N. D., 2001, PASP, 113, 821

Richardson, N., A Five–Year Spectroscopic and Photometric

Campaign on the Supergiant Star Deneb, M.S. Thesis, 2006

Kaufer et al. 1996, A&A, 305, 887

Kunasz, P. B., Morrison, N. D., Spressart, B. 1983, ApJ, 266, 739

Morrison, N. D., & Gordon, K. D., 1996, Bull. AAS, 27, 1312

Przybilla, N. et al., 2004, Proceedings IAU Symposium No. 224, DOI:

10.1017/S174392130400482XRosendhal, J., D., 1973, ApJ, 186, 909Stahl et al. 1995, Jour. Astr. Data 1, No. 3

Straizys, V, & Laugalys, V, 2007, Baltic Astronomy, 16, 167

Talavera, A. & Gomez de Castro, A. I., 1987, AA,181, 300T

REFERENCES