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Orion Constellation

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Atacama Compact Array (ACA): 12m×4 + 7m×12 East-Asian (EA: JP+TW+KR) contribution

Main Array: 12m×50

North-American (NA: US+CA +TW) + European (EU) contribution

ALMA = Atacama Large Millimeter/submillimeter Array

Largest array telescope ever built. Inaugurated on 2013-03-13

=>TW has open access to EA and NA times by proposals!!

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ALMA Array Operation Site-5000m

One of the Driest places

Remote Observing

Operation Support Facillity (OSF, 2900m)

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Birdview of ALMA

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ALMA vs. Hubble Space Telescope

NIR-Optical-UV

Radio

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grthjo

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E N ?RUTa HJa ^RN NM J 3 JLJVJ

( ,

Credit ALMA

~ 200 billion stars, and our Sun is one of them!!

Stars like our Sun form and die anytime, anywhere!! How and Why?

Habitable Exoplanets?? Extraterrestrial Lifes? Origin of Lifes?

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?RUTa HJa JWM D UJ Da NV

Harvey Resources

Most stars seem to have planetary systems, like our solar system.

& Ua0 ( (. J

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ESO Copyright Conditions

Proxima Centauri b exoplanet Habitable? Not clear yet.

Proxima Centauri

Alpha Centauri Binary

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Orion Constellation

Credit: W.-H. Wang

Tobin et al.

100 pc

Tahani et al. 2019

M42

& L0( Ua

0 J

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D UJ Da NV NWLU NM RW J UJ PN A 5U M1

& J c Lc& Ua1

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D J JWM BUJWN 8 VJ R W B LN

12

5 V URLJ NM Ka ?JPWN RL ORNUM 3WP UJ V VNW V W JMMR R W!

&   5 W N ^J R W O 3WP UJ ? VNW V è HJa

V L 3WP UJ ? VNW V W N J KN K W   5 W N ^J R W O ?JPWN RL OU è HJa V L

?JPWN RL 8U W N J KN K W

? N ^N !

?JPWN RL K JTRWP LJW N^NW J J RWP MR T O V

O VRWP J WM N J

@N J R W

"J R

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Magnetic Braking Catastrohe (MBC) Collapse of Magnetized Rotating Core

(B-axis // J-axis, Ideal MHD, field frozen in material)

Allen et al. 2003

No rotating disk formed inside Flattened EnvelopeèMagnetic Braking Catastrohe (MBC)

Extended Infalling envelope Hour-glass B-field morphology

Flattened Envelope (Pseudodisk)

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:: && J "O VRWP NPR W 2& Ua RW BN N 5U M

Hirano et al. 2006 Wiseman et al. 2001 Optical image by

Patrick Hochleitner

3PNc& ) a ! VRW R ac ( W! ?c - ? W

core

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NH3 Core is rotating (r ~ 0.05 pc)

Lee et al 2009

Rotating Disk found!

rD ~15 au è M ~ 0.08 M¤ Gravitational

collapsing+Rotating C18O Envelope

(Pseudodisk) r ~ 400 au

Cont + C18O SO Disk Wind

J-axis

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NH

3

Core 8UJ NWNM

Matthews et al. 2009

?R JURPWVNW KN

4"J R JWM C J R W "J R

WR RJU D L N

50000 au

B J-axis

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Rotating Core

Matthews et al. 2009

B-field in inner region (pseudodisk) from ALMA dust polarization at 230/345 GHz

1.  Misalignment betw core & pseudodisk & disk 2.  Field guided infall forming Pseudodisk!

3. Pseudodisk has a pinched field morphology due to gravitational infall mainly along equatorial plane and a toroidal field produced by rotation!

Bϕ ~ 7.8 mG at r ~ 100 au 4. Disk field?? Unresolved!

B

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DRA RWN B UJ RbJ R W1

DRA N H2 N A OU in HH 211

Lee et al 2018b, Nature Comm.

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3PN c & ) a !

? c ? W

A R W

6NN Ua 7VKNMMNM

B J

VLT image at 0.34 resolution McCaughrean et al. 2002

:: & : N

@:( 5 N

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6R T O WM R 3 ?3 () 9:b 2 -J N U R W 6c) J

Lee et al. 2017a, Science Advances

: 5A DRA

@:(

7MPN" W 6R T " :JVK PN

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WWN V DRA N R RW & J / N J R W

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3LL N R W JWM 7SNL R W B LN N

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Orion Constellation

HH 111 @ 0.5 Myrs, M ~ 1.5 Ms

32000au (~0.5 light-year)

B-axis // J-axis è MB?

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(1)  Extended Perpendicular to the jet (2)  Rotating-collapsing inner core (3)  Mass ~ 0.3 Ms

(4)  Infall rate ~ 4.3e-6 Ms yr

Gaseous Envelope in C

18

O J=2-1 (Lee 2010, 2011)

Keplerian rotating disk rD ~160au!!

è M ~ 1.5 Msun è Age ~ 0.5 Myr old

7200 AU

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(1)  Extended Perpendicular to the jet (2)  Rotating-collapsing inner core (3)  Mass ~ 0.3 Ms

(4)  Infall rate ~ 4.3e-6 Ms yr

Gaseous Envelope in C

18

O J=2-1 (Lee 2010, 2011)

7200 AU

Lost of angular momentum at 2000 AU (5”) results in a small disk. Magnetic Braking (MB)?

(Lee 2010, 2016)

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Lee et al. 2020, Nature Astronomy First spiral arms detected in active accretion phase

because of ALMA unprecedented resolution!!!

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=N UN RJW C J RWP 3LL N R W 6R T

C J R W GNU LR a G 0 9? C I &

0 C G 0 9 ? C I & è VJUUN 2 VJUUN JMR

è WNNM JW J Ja J M! K 1

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Tomida et al. 2017 Spirals Repeatedly Formed by Gravitational Instability

sustained by envelope accretion

Gravitational Torque can transport angular momentum outwards.

è Material can accrete and fall inwards.

è Solution to the long-standing angular momentum problem in disk accretion.

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Formation Process of a Solar System like our own

1.  Infall guided by magnetic field, forming flattened envelope 2.  Keplerian disk formed in flattened env. feeding protostar 3.  Magnetic braking may reduce the disk size, if J // B-axis

4.  Jet magnetized, launched from the innermost edge of disk.

5.  GI induces spiral arms transporting L inside Keplerian disk.

Disk Wind carrying away L from the disk? MRI turbulence?

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6R T N RW N 7J Ua B J N O D J 8 VJ R W

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: EJ 2 c & ?a R M

c ?

¤

ALMA (ESO/NAOJ/NRAO), ESA/Hubble and NASA N

:DE RVJPN 3 ?3 4 PJW N JU &

Protoplanetary Disk

32 AU

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: EJ B UJWN J a 6R T ^ D UJ Da NV

@N WNe( 3F

ALMA (ESO/NAOJ/NRAO)

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ALMA (ESO/

NAOJ/

NRAO)Andrews et al.; N. Lira

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EH :aM JN 2 & ?a R M

c ?

¤

S. Andrews (CfA), B. Saxton (NRAO) ALMA (ESO/NAOJ/NRAO) 22 au gap

Protoplanetary disk

1 au gap

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PDS 70

ALMA (ESO/NAOJ/NRAO), ESA/Hubble and NASA/Andrea Isella et al

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4JKa J

BUJWN O VNM KNRWP O VNM

6 RWP 2&( J

= R N 4NU d

:DE

ALMA (ESO/NAOJ/NRAO) 3 ?3

8 VJU J 6NK R 6R T 2 )) 4a M

& .?

¤

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D UJ Da NV 2 ) 4a

Image Credit: Harvey Resources

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DRV UJ R W O BUJWN 8 VJ R W

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3Wa URON K RUMRWP KU LT RW :JVK PN d

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5 V UN A PJWRL ? UNL UN 5A? O WM RW 6R T 3 V

nfum v G 0 9? C I &

è sp y c

Lee et al. 2017b iz y

~kl

l lwx

~kl l

Keplerian Rotation è M ~ 0.25 Msun

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Disk Atmosphere in Complex Organic Molecules

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More COMs found in Disk Atmosphere

Lee et al. 2019a

The abundance ratios of these molecules are also similar to those in Comet Lovejoy è Carried over to the protoplanetary disk??

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3 O 5 VN ^NS a JTNW O V @J R WJU D JLN D J R W W && & &

J OR MR L ^N NM Ka JW 3 JURJW JVJ N J W VN

^NS a W && && , R J N R MRL L VN

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?N JW Ul JU O WM RW EH :aM JN UJWN J a MR T

Catherine Walsh ALMA (ESO/NAOJ/NRAO)

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Herbst & van Dishoeck 2009

5 UM JWM 6NW N

? UNL UJ 5 N

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è Amino acids è Aliens ?

Complex Organic Molecules (COMs)

參考文獻

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