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Transients in the Local Universe

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Transients in the Local Universe. Mansi M. Kasliwal (Caltech) On behalf of the PALOMAR TRANSIENT FACTORY The Eventful Universe March 18, 2010. Why “Local” Universe?. Gravitational Waves: d < 200Mpc. UHECR, GZK Cutoff ~100 Mpc. Neutrinos: d < 10Mpc. Empty?. Which “Transients”?. - PowerPoint PPT Presentation
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Transients in the Local Universe Mansi M. Kasliwal (Caltech) On behalf of the PALOMAR TRANSIENT FACTORY The Eventful Universe March 18, 2010
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Page 1: Transients in the Local Universe

Transients in the Local UniverseMansi M. Kasliwal (Caltech)

On behalf of thePALOMAR TRANSIENT FACTORY

The Eventful UniverseMarch 18, 2010

Page 2: Transients in the Local Universe

The Eventful Universe/ Kasliwal 2

Why “Local” Universe?

Mar 18, 2010

Gravitational Waves: d < 200Mpc

UHECR, GZK Cutoff ~100 MpcNeutrinos: d < 10Mpc

Page 3: Transients in the Local Universe

The Eventful Universe/ Kasliwal 3

Empty?

Mar 18, 2010

Which “Transients”?

Page 4: Transients in the Local Universe

The Eventful Universe/ Kasliwal 4

The Experiment

~20,000 galaxies with d < 200 Mpc (RARE) 1-day cadence (FAST) m < 21 depth (FAINT) Real-time discovery pipeline Built-in photometric follow-up Spectroscopic classification of ALL candidates

Mar 18, 2010

To find transients in the gap, PTF is the most sensitive survey thus far….

Page 5: Transients in the Local Universe

The Eventful Universe/ Kasliwal 5

2008ha in 2002cx-family? 2002cx-family: “peculiar” Ia as

standard candle deviants 2008ha:

>10x fainter >30 days shorter lived >3000 km/s slower ejecta

White Dwarf OR Massive Star?

Mar 18, 2010

Foley et al. 09

Valenti et al. 09

Page 6: Transients in the Local Universe

The Eventful Universe/ Kasliwal 6

Result I: Origin of 2002cx-family

Mar 18, 2010

PTF09eoi bridges the gap between 2008ha and 2002cx PTF09ego is the brightest member of this class

If Ia, Mej > 4.5 M! NOT a white dwarf Are these massive stars, perhaps collapsing into a black hole?

Page 7: Transients in the Local Universe

The Eventful Universe/ Kasliwal 7

Background: 2005E

Mar 18, 2010

Halo Location: Not a Massive Star

Fast Photometric EvolutionFaint LuminosityLowest Known EjectaAIC or SN .Ia?

Perets et al. 09Perets et al. 09

Page 8: Transients in the Local Universe

The Eventful Universe/ Kasliwal 8Mar 18, 2010

Result II: Mysterious PTF09davLocation:

40kpc from putative spiral hostPhotometric Evolution:

In the GAP, Mg = -14.8 Very fast, 1 mag in 10 days Very red, g-r = 1.2

Spectrum: Similar to SN1991bg but with He Hydrogen in nebular phase

Page 9: Transients in the Local Universe

The Eventful Universe/ Kasliwal 9

Result III: Ephemeral PTF10bhp

Mar 18, 2010

Very short-lived? t1 = 5 days

Subluminous Mr = -16

Spectroscopically, Type Ic

Page 10: Transients in the Local Universe

The Eventful Universe/ Kasliwal 10

Stay tuned…The fun has only just begun!

Mar 18, 2010

Summary:1. New members of the 02cx-family:Evidence for a massive star origin2. The mysterious, faint, fast

PTF09dav3. The short-lived PTF10bhp

Page 11: Transients in the Local Universe

The Eventful Universe/ Kasliwal 11

Extra slides…

Mar 18, 2010

Page 12: Transients in the Local Universe

The Eventful Universe/ Kasliwal 12Mar 18, 2010

Bright, Plenty

Faint, Rare

Page 13: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 13Aug 17, 2009

Theoretical Impetus

Bildsten et al 07

Kulkarni 05

e.g.

, Fry

er e

t al 2

007

AICMetzger et al 09

Page 14: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 14Aug 17, 2009

Predicted Light Curves

Metzger et al. 09Fryer et al. 09

AIC

Fryer et al. 09

Fallback BH

Fryer et al. 09

.Ia

Page 15: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 15Aug 17, 2009

Kasliwal et al, in prep

eLIGO -> PTF

• LIGO localizations are very poor– 50%ile : 7..40 sq deg– 90%ile : 120..700 sq deg

• If follow-up is concentrated on known galaxies within 50 Mpc, foreground/background false positives are reduced to tens to hundreds of arcmin!

Page 16: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 16Aug 17, 2009

A 200Mpc Catalog

• Left : Completeness of compiled galaxy catalog given expected total light (Schechter function) vs. distance

• Right : Completeness as a function of depth of survey. Major surveys contributing to nearby galaxy measurements are denoted by vertical lines with length proportional to fraction of sky covered.

Page 17: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 17Aug 17, 2009

P60-M81OT-071213 : Faint, Fast Nova?

• Discovery by P60-FasTING on UT 2007 Dec 13, Mg = -7.3• Too fast declining (1 mag day-1) for its faintness• Width of Balmer emission lines, 3100 km s-1, 2400 km s-1

• H/H = 3.8 => Av = 0.85 • No X-ray emission a week after peak : Not a NS/BH

Kasliwal et al, in prep

Page 18: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 18Aug 17, 2009

P60-M81OT-081203 - Featureless?

• Photometrically like a nova, -7.6• Spectroscopically featureless! • Foreground? Background? • Novel? Synchrotron?

Kasliwal et al, in prep

Page 19: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 19Aug 17, 2009

M85OT : A Luminous Red Nova

• MR = -12! Extremely red (g-R = 2) and long plateau at 2 x 1040 ergs/s

• FWHM H = 350 km/s, Teff ~ 4700K• Proposed Models:

– Stellar Merger (Soker & Tylenda 2006, M2/M1 ~ 0.03..0.1, cool remnant) – Extreme Classical Nova (Shara, low-mass WD with hot remnant)– Extreme Type IIp supernova (Pastorello et al 2007)

• Rate : >0.015 / yr / 1011 Lsun

Kulkarni et al. 2007

Page 20: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 20Aug 17, 2009

“eAGB” stars

• SN2008S (in NGC6946) and NGC300-OT had extremely red progenitors - dust enshrouded SNe? e-capture SNe?• Spectroscopic and Photometric explosion signature - LBV?

Thompson et al 2008 Smith et al 2008

Page 21: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 21Aug 17, 2009

Woosley et al 2002

Page 22: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 22Aug 17, 2009

I. P60-FasTINGNov 18 Reference Subtraction

Page 23: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 23Aug 17, 2009

Faint and Fast Novae

Kasliwal et al. 2009

Page 24: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 24Aug 17, 2009

MMRD?

Kasliwal et al. 2009

Page 25: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 25Aug 17, 2009

II. CFHT-COVET

Page 26: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 26Aug 17, 2009

CFHT-COVET• 7 sq deg Virgo + 3 sq

deg Coma, daily, 56 days

• 160 Transients : – 140 Background

SN/AGN – 20 Virgo Novae

• Upper limit : – @ Mv < -9, Rate < 9.5 x

1010 Lsun-yr– @ Mv < -13, Rate < 4.4 x

1011 Lsun-yr

Page 27: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 27Aug 17, 2009

Mystery III. 2008S/NGC300-OTWhat type of star exploded !?

8-11 M e- capture?

Thompson et al. 2008, Prieto et al. 2008

>20 MLBV

Smith et al. 2009

12-25 M SN?

Gogarten et al. 2009

Page 28: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 28Aug 17, 2009

Mystery IV. M85OT/M31RV/V838Mon

Thompson et al. 2008, Prieto et al. 2008

• MR = -12! Extremely red (g-R = 2) and long plateau at 2 x 1040 ergs/s• Late-time (180 days) excess in Spitzer mid-IR bands similar to V838Mon and M31RV ;

Blackbody Teff ~ 950K (Rau et al. 2006)• FWHM H = 350 km/s, Teff ~ 4700K• Proposed Models:

– Stellar Merger (Soker & Tylenda 2006, M2/M1 ~ 0.03..0.1, cool remnant) – Extreme Classical Nova (Shara, pers comm)– Extreme Type IIp supernova (Pastorello et al 2007)

Kulkarni et al. 2007

Page 29: Transients in the Local Universe

Stellar Death and Supernovae / Kasliwal 29Aug 17, 2009

Local Overdensity


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