Mapping Supermassive Black Hole Winds, from the Event Horizon up to Galaxy...

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Mapping Supermassive Black Hole Winds, from the Event Horizon up to Galaxy Scales “X-ray Skies with High-Res Eyes: Imaging the Cosmos with AXIS” Carnegie Institution for Science, Washington, DC 6-7 August 2018 Francesco Tombesi

Transcript of Mapping Supermassive Black Hole Winds, from the Event Horizon up to Galaxy...

Page 1: Mapping Supermassive Black Hole Winds, from the Event Horizon up to Galaxy …axis.astro.umd.edu/images/Tombesi.pdf · 2018. 8. 8. · Mapping Supermassive Black Hole Winds, from

Mapping Supermassive Black Hole Winds, from the Event Horizon up to Galaxy Scales

“X-ray Skies with High-Res Eyes: Imaging the Cosmos with AXIS”

Carnegie Institution for Science, Washington, DC

6-7 August 2018

Francesco Tombesi

Page 2: Mapping Supermassive Black Hole Winds, from the Event Horizon up to Galaxy …axis.astro.umd.edu/images/Tombesi.pdf · 2018. 8. 8. · Mapping Supermassive Black Hole Winds, from

(Kormendy & Ho 2013)

Relations Between SMBHs and Host Galaxies?M

BH(M

¤)

σ (km/s)

(Bower et al. 2012)

No AGN feedback

With AGN feedback

log(Stellar Mass/h-1 M¤)

Gal

axy

Stel

lar M

ass

Func

tion

l SMBH radius is >109 smaller than host galaxy

l SMBH mass is <1% stellar bulge mass

l SMBH gravitational energy > binding energy galaxy bulge!

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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Ultra-Fast Outflows (“UFOs”)

(Pounds et al. 2003)

NGC 4051 v~0.1c

(Tombesi et al. 2015, Nature)

(Reeves et al. 2009)

PDS 456 v~0.25c

Rest-frame energy (keV)

Rat

io s

pect

rum

/mod

el IRAS F11119 v~0.25c

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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(Ohsuga et al. 2009)

Are Winds at SMBH- and Galaxy-Scales Related?

(Wagner et al. 2013)

SMBH Winds(< 1pc scales)

Galactic Winds (~kpc scales)

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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Galaxy-Scale Molecular Outflow

• IRAS F11119+3257, ULIRG z=0.189, QSO luminosity 1046erg/s

• Herschel spectrum OH 119µm P-Cygni line profile (Veilleux et al. 2013)

• Molecular outflow 1000 km/s, 800 M¤ yr−1 at >300 pc

• Follow-up of CO outflow with ALMA (Veilleux et al. 2017)

Velocity (km/s)

Flux

den

sity

(Jy)

(credit ESA press release)

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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Galaxy-Scale Molecular Outflow

• IRAS F11119+3257, ULIRG z=0.189, QSO luminosity 1046erg/s

• Herschel spectrum OH 119µm P-Cygni line profile (Veilleux et al. 2013)

• Molecular outflow 1000 km/s, 800 M¤ yr−1 at >300 pc

• Follow-up of CO outflow with ALMA (Veilleux et al. 2017)

Velocity (km/s)

Flux

den

sity

(Jy)

(credit ESA press release)CO emissionALMA

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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• Long 250ks Suzaku observation in May 2013

• Detection (6.5sigma) broad absorption line at rest-frame E=9.82keV

• XSTAR fit: v=0.255c, logxi=4.11, Nh=6�1024, covering fraction >0.85

• Follow-up with NuSTAR (Tombesi et al. 2017)

X-ray Ultra-Fast Outflow

Rest-frame energy (keV)

Rat

io s

pect

rum

/mod

el

(credit ESA press release)

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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• Long 250ks Suzaku observation in May 2013

• Detection (6.5sigma) broad absorption line at rest-frame E=9.82keV

• XSTAR fit: v=0.255c, logxi=4.11, Nh=6�1024, covering fraction >0.85

• Follow-up with NuSTAR (Tombesi et al. 2017)

X-ray Ultra-Fast Outflow

Rest-frame energy (keV)

Rat

io s

pect

rum

/mod

el

(credit ESA press release)

Rest-frame energy (keV)

Rat

io s

pect

rum

/mod

el

NuSTAR

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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(credit NASA/GSFC)(Credit: NASA/GSFC)

Galaxy-Scale Feedback from AGN Winds?

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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(Gaspari & Sadowski 2017)

Self-Regulation of SMBH Feeding and Feedback

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ξ ∝ r−0.58 NH ∝ r−0.44

vout ∝ r−0.40

M•

out ∝ r0.16

P•

out ∝ r−0.22 E•

K ∝ r−0.60

Log(r)

Log(r)

Log(r)

Log(r)

Log(r)

Log(r)

Log(ξ)

Log(v out)

Log(P out)

Log(NH)

Log(Mout)

Log(EK)

(Tom

besi

et a

l. 20

13)

UFOWA

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ξ ∝ r−0.58 NH ∝ r−0.44

vout ∝ r−0.40

M•

out ∝ r0.16

P•

out ∝ r−0.22 E•

K ∝ r−0.60

Log(r)

Log(r)

Log(r)

Log(r)

Log(r)

Log(r)

Log(ξ)

Log(v out)

Log(P out)

Log(NH)

Log(Mout)

Log(EK)

(Tom

besi

et a

l. 20

13)

UFOWA

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Multi-phase/Multi-scale Wind Feedback

(NG

C 41

51, W

ang

et a

l. 20

10)

Multiwavelength campaigns with ALMA, VLT, E-ELT, GMT, …: hot/cold gas mixing, AGN wind power, wind bubbles, shocks, photoionization cones, outflow morphology, AGN/star formation comparison, …

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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Direct Imaging of Galactic Winds with AXIS

(AXIS Team)NGC 3079

F. Tombesi – Imaging the Cosmos with AXIS, Washington DC, 6-7 August 2018

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Thank you for your attention!

Active Galaxy

Wind

Supermassive Black Hole

Jet