Variability of Accreting White Dwarf Binaries and Other Compact Objects
Manuel Pichardo Marcano
Texas Tech University
Thomas J. Maccarone & Liliana Rivera Sandoval
Compact Binaries Surveys
1- SCOVaS: Survey for Compact Objects and Variables
Pichardo Marcano et al. (2021a)
Pichardo Marcano et al. (in prep.)
2- TACOS: TESS AM~CVn Outbursts Survey
Pichardo Marcano et al. (2021b)
Compact Binaries Surveys
X-ray unbiased search
SCOVaS: Survey for Compact Objects and Variables Stars
- HST Archive
- 7 Globular Clusters
- Many Exposures
- Different properties
- Metallicity
- Core-collapsed
- Non core-collapse
SCOVaS: Survey for Studying Compact Objects and Variables
- Focus: Cataclysmic Variables (CVs) with HST
- First Unbiased Survey for CVs in Globular Clusters
- X-ray faint CVs
- Orbital Periods
- Spatial Distribution:
- Looking at the dense Core of Clusters
- Next: Search in the Outskirts
- Optical Counterpart X-ray/Radio Sources in GCs
Preliminary Results
NGC 6397
- WFPC-2
- March-April 2005:
- 126 orbits
- F814W, F606W and F336W
- Exp time: 500-700 s
Preliminary Results
NGC 6397
- WFPC-2
- March-April 2005:
- 126 orbits
- F814W, F606W and F336W
- Exp time: 500-700 s
A new candidate Redback Pulsar
HUGS catalogue. (Piotto et al. 2015, Nardiello et al. 2018)
Pichardo Marcano et al. (2021a)
X-ray
HST F336W
Radio
Zhao et al.(2020)
Zhao, [...], Pichardo Marcano, et al. (2020)
A new candidate Redback MSP
Pichardo Marcano et. al (2021a)
- Porb 1.96 days
- Longest Porb for Redback in GCs
- Missed MSP in Pulsar Searchers
Light Curves Known CV Candidates
High and Low state?
Novalike?
Pichardo Marcano et. al (in prep)
New Eclipser?
Light Curves Known CV Candidates
Pichardo Marcano et. al (in prep)
New CV Candidate
Pichardo Marcano et. al (in prep)
New CV Candidate
- New CV Candidate
- Not Detected X-rays
- Potential Porb
-
5.21 hours
-
Pichardo Marcano et. al (in prep)
NGC 6397
- Pipeline to find interesting objects:
- CMD Position and Periodicity/Variability Searches
- We were able to recover all known CV Candidates
- Found Orbital Period Redback Pulsar
- Potential New, X-ray faint, CV Candidate
- Many more variables to analyze...
Preliminary Results
M 92
- WFPC-2
- 2008-01-25 to 2008-01-30:
- 76 Exposures
- F555W
- Exp time: 10 s
M 92
HST vs Ground-based
Yepez et al. (2020)
Ground-based Data
HST Data
New Variables in the Core
SX Phe
- Good Distance indicator:
- Strong P-L relation
- Less common than RR Lyrae
-
Blue Straggler
- Product of Binary evolution
P = 1.38 hr
Pichardo Marcano et. al (in prep)
M 92
- New variables in the core:
- SX Phe, RR Lyrae, AB, ....
- Search for Optical Counterparts of X-ray sources:
- 1 Pulsar, 4-5 CVs
- Many more variables to analyze...
-
Precursor
- TESS (Duffy et al. 2021)
- GOTO data
- Echo Outbursts
- DIM with EMT (e.g. Hameury & Lasota 2021)
TESS AM CVn Outbursts Survey
Pichardo Marcano et al. (2021)
Outbursts
Pichardo Marcano et al. (2021)
PTF1 J0719+4858:
-
Similar to Dwarf Novae:
- Hameury et al. (2020)
- Rivera Sandoval et al. (2021)
Color Evolution
Pichardo Marcano et al. (2021)
Long-term monitoring
Pichardo Marcano et al. (2021)
- Orbital Periods:
- 2-minute cadence
- Limits on Recurrence Time
- "Normal Outburts"
SO durations vs Porb
Pichardo Marcano et al. (2021)
Other work with Accreting WDs
-
Follow-up eROSITA transient:
- TESS time series analysis
-
-
Atel: Pichardo Marcano (2020)
-
Paper: Schwope, [...], Pichardo Marcano, et al. (2021)
-
Caltech
Summary
- GOTO:
- Time-domain astronomy
- ZTF, ATLAS, TESS, HST
- Experience Transients
- Expand my expertise
- Time-domain astronomy
- Common interest with Warwick Scientists
- Compact Binaries:
- Accreting WDs
- Compact Binaries:
- Experience Spectroscopy:
- IFU: MUSE, VIMOS
- GEMINI
Extra Slides
TACOS Summary
-
Precursors and "Normal" Outbursts:
- Relatively Common
- Short Duration (missed ground-based)
-
Echo Outbursts:
- Different morphology
- Enhanced Mass Transfer
- SO durations overestimated
- Two new candidate periods
- Color Evolution
Long-term monitoring
Pichardo Marcano et al. (2021)
- Orbital Periods:
- 2-minute cadence
- Limits on Recurrence Time
- "Normal Outburts"
Outbursts
Pichardo Marcano et al. (2021)
Transiting Exoplanet Survey Satellite (TESS)
Caltech
-
Porb 20 to ~ 60 minutes (?)
-
Superoutburts (SO) and "Normal" outbursts (NO)
-
SO: Superhumps (periodic brightness variation )
-
-
Disk instability model (DIM)
-
Constant Mass transfer rate
-
Tidal-thermal disk instability model
-
Outbursting Systems
Empirical Relationships
- Trec prop Porb^7.35
- Tdur prop Porb^4.54
- Delta mag prop Porb
- Long-term
- Ground-Based:
- PTF
- CRTS
Levitan et al. 2015
See also Duffy et al. 2021
InterviewWarwick
By mmarcano22
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