2s · ... “Origins of Absorption Systems of Classical Nova ... X b « >&multiple gas shell ......

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2016 ᖺᗘ◊✲ᡂᯝሗ࿌᭩ : ᪩ᮇῶගᮇV2659 Cyg ࡅ࠾྾⥺㛫ኚ㉳※ ᢸᙜ: Ἑ⚽ୡ ඹ◊✲⪅㸸 Ashish RajIndian Institute of Astrophysics, India㛵㐃ฟ∧: Akira Arai, Hideyo Kawakita, Yoshiharu Shinnaka, Akito Tajitsu, 2016, Astrophysical Journal, 830, 30, “Origins of Absorption Systems of Classical Nova V2659 Cyg (Nova Cyg 2014)” 㛵㐃ᏛⓎ⾲➼: V2659 Cyg (=Nova Cyg 2014) ྾⥺㉳※᪥ᮏኳᏛ 2016 ᖺᏘᖺ - 29 -

Transcript of 2s · ... “Origins of Absorption Systems of Classical Nova ... X b « >&multiple gas shell ......

Page 1: 2s · ... “Origins of Absorption Systems of Classical Nova ... X b « >&multiple gas shell ... (Williams et al. 2008; Williams & Mason 2010; Williams 2013 ...

2016

: V2659 Cyg

:

Ashish Raj Indian Institute of Astrophysics, India

:

Akira Arai, Hideyo Kawakita, Yoshiharu Shinnaka, Akito Tajitsu, 2016, Astrophysical Journal,

830, 30, “Origins of Absorption Systems of Classical Nova V2659 Cyg (Nova Cyg 2014)”

:

V2659 Cyg (=Nova Cyg 2014)

2016

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V2659 Cyg

Ashish Raj Indian Institute of Astrophysics, India

V2659 Cyg

V2659 Cyg

double-horned

1

1.1

108 K (Thermo-Nuclear Runaway: TNR)

TNR

free-free

P Cyg

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1950 McLaughlin

McLaughlin 1950a, 1950b, 1965 McLaughlin

”pre-maximum” ”principal” “diffuse enhanced” “Orion”

multiple gas shell

”pre-maximum”

”principal” ”pre-maximum”

”diffuse enhanced” ”Orion” ”principal”

McLaughlin

1.2 Transient Heavy Element Absorption (THEA)

LVC (Low-Velocity Component) HVC (High-

Velocity Component) LVC Williams et al. (2008) Williams

(2013) (Transient Heavy Element Absorption:

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THEA)

[THEA ]

McLaughlin ”principal”

2~8

v = 500 km/s — 1000 km/s LVC

Fe II, Ti II, Na I, Cr II, Zr II, Sr II, V II, Y II, Ca II

< 4 eV

e.g.,

Weaver 1944; Kogure & Leung 2007 He I, Fe II, O I

80%

McLaughlin (1965) Nova Gem 1912 principal

THEA

HVC LVC 2 LVC

(Williams et al. 2008; Williams & Mason 2010; Williams 2013; Arai et al.

2016) LVC 1000 km/s — 1500 km/s

LVC

LVC

HVC

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1.3

1 Li et al. (2017)

Mason et al. (2018)

Williams (2013) THEA Fe II

He/N

Williams LVC

THEA

LVC 7Be τ 53 Williams (2013)

Li et al. (2017)

1.4 1.5

1.

THEA 7Be

Williams (2013)

Li et al. (2017)

Mason et al. (2018)

1.4 Multiple ejection model

Li et al. (2017) Chomiuk et al.

2014 20%

Derdzinski et al. 2017 THEA

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L2

Fe Fe II Fe III

~1000 km/s THEA

Williams (2013) LVC

LVC Li et al.

(2017) Williams (2013)

7Be

(Tajitsu et al. 2016; Molaro et al. 2016) 7Be 537Li 7Be

Tajitsu et al. (2015) Tajitsu et al. (2016) Molaro et

al. (2016) 100

LVC HVC V339 Del 7Be

LVC HVC V5886 Sgr, V2944 Oph7Be LVC

HVC THEA

Williams 2013

Li et al. (2017)

1

1.5 (Single ejection model)

Li et al. (2017) Mason et al. (2018) (

) ballistic ejecta

ballistic law Habble flow (v r)

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Shore (2012) T Pyx

Mason et al. (2018) Shore (2012)

LVC HVC

Mason et al. (2018) TNR

1.6

LVC HVC

Mason et al. (2018)

Li et al.

(2017)

T Pyx

Uthas et al. 2010 0.7M

LVC HVC

L2

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slow novae fast novae LVC

2014 V2659 Cyg

(Arai et al. 2016)

(Arai et al. 2016)

Li et al. (2017) Mason et al. (2018) Arai et al.

(2016)

LVC HVC

2 V2659 Cyg

2014 3 V2659 Cyg ( 2014)

Miyaki Observatory

Fe II

420 – 860 km/s 1 V2659 Cyg

Strope et al. (2010) jitter

3

HDS Noguchi et al. 2002 BOAO

BOES Kim et al. 2007

BOES WINERED Ikeda et al. 2016

2 BOES

Ashish Raj

.

(UT) t [ ] [ ]

2014/05/01 21 1200 27,000 BOES

2014/05/13 33 1200 27,000 BOES

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(UT) t [ ] [ ]

2014/05/01 21 1200 27,000 BOES 2014/05/22 42 600 72,000 HDS

2014/06/15 66 1200 27,000 BOES

2014/09/21 164 1200 27,000 BOES 2014/09/27 170 4,400 28,000 WINERED

t=0

V2659 Cyg HDS BOES WINERED

4

4.1

/HDS (t=33 d)

Arai et al. (2016) Arai et al. (2016) He I

Fe II Ti II, Cr II H I Fe II

(LVC) (HVC) v= 620 km/s v= 1300 km/s

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Arai et al. (2016) t=33d

BOAO/BOES t=21d, t=42d, t=66d t=169d, 170d

3.5 2 V2659 Cyg

Fe II 5018

HDS BOES

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LVC HVC Fe

II 5018

4.2 LVC HVC

Fe II 5018 Na I D 5899 LVC HVC

LVC HVC

fitting

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Fe II 5018 Na I D 5899 LVC HVC

LVC HVC

Na I D 5899 0.0 eV

Fe II 5018 10.3eV

LVC HVC

filling-factor 1

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Arai et al. (2016)

Fe II gf

LVC HVC

LVC HVC

L2

a few revolutions?

Li et al. (2017)

(nova wind)

Li et al. 2017

ballistic

flow (Prialnik1986)

Mason et al. 2018 ballistic

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t=33d gf

4.3 HVC

LVC HVC

HVC

HVC

Shore (2012) Mason et al. (2018) moving ionization front

2011 T Pyx

Shore (2012) T Pyx Shore (2012)

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HVC

HVC t=21d

t=33, 42, 66 d

HVC

v r

(r) r / vmax t ,

Fe III, Fe II, Fe I

(Tph)

UV X Fe II

Fe III

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Fe II

1—5

Fe II 1—4

Fe III 1 2

F2+ Fe II

HVC

HVC

Mason et al. (2018) V1309 Cen UV C N

filling factor Mason

et al. 2018 LVC HVC

HVC

Mason et al. (2018)

filling factor

t (d) t (d)

Vm

in (k

m/s

)

Vm

ax (k

m/s

)

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filling factor

HVC

ballistic flow

HVC

4.4 LVC

HVC

LVC

LVC LVC HVC

LVC

HVC

FWHM HVC

Arai et al. (2016) t= 33d LVC

optically thick wind LVC 4.2

THEA 80%

80%

Williams & Mason 2010

v (r / vmax × t)

(We can observe)

Fe II

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Williams et al. (2008) Williams (2013) LVC

Li et al. (2017) L2 TNR

LVC HVC

53 7Be Li et al. (2017)

Mason et al. (2018) LVC HVC

Mason et al. (2018) LVC HVC

Williams

LVC HVC

LVC HVC

LVC HVC

LVC

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4.5

[O I] [O III] He I 10830 600 km/s

+400 km/s

He I 10830

FWHM 900 km/s t=66d LVC

FWHM 1700 km/s HVC

( 1600 km/s) Mason et al. (2018)

Mason et al. (2018)

Mason et al. (2018)

V2659 Cyg

biconical

structure

V2659 Cyg HVC

LVC

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He I

5

LVC

HVC V2659

Cyg ( 2014)

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Mason et al. (2018) 1

Mason et al. (2018)

MMRD7Be Li et

al. (2017)

LVC

LVC

HVC

Mason et al. (2018)

Arai, A., Kawakita, H., Shinnaka, Y. & Tajitsu, A. 2016, ApJ, 830, 30

Chomiuk, L., Linford, J. D., Yang, J., 2014, Natur, 514, 339

Derdzinski, A.M., Metzger, B.D., Lazzati, D., 2017, MNRAS, 469, 1314

Ikeda, Y., Kobayashi, N., Kondo, S., et al., 2016, SPIE, 9908, 5

Kim, K., Han, I., Valyavin, G. G., et al., 2007, PASP, 119, 1052

Kogure, T., & Leung, K.-C. (ed.) 2007, The Astrophysics of Emission-Line Stars (Vol. 342;

Berlin: Springer)

Li, K., Metzger, B., Chomiuk, L., et al. 2017, NatAs, 1, 697

Molaro, P., Izzo, L., Mason, E., Bonifacio, P., Della Valle, M., 2016, MNRAS, 463, 117

Mason, E., Shore, S. N., D. G. Aquino, I., Izzo, L., Page, K., Schwarz, G. J., 2018, ApJ, 853, 27

McLaughlin, D. B., 1950a, PA, 58, 50

McLaughlin, D. B., 1950b, PASP, 62,185

McLaughlin, D. B., 1965, POMic, 9, 113

Noguchi, K., Aoki, W., Kawanomoto, S., et al., 2002, PASJ, 54, 855

Prialnik, D., 1986, ApJ, 310, 222

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Shore, S. N. 2012, Bulletin of the Astronomical Society of India, Vol. 40, p. 185

Strope, R. J., Schaefer, B. E., Henden, A. A., 2010, AJ, 140, 34

Tajitsu, A., Sadakane, K., Naito, H., Arai, A., Kawakita, H., Aoki, W., 2015, Natur, 518, 381

Tajitsu, A., Sadakane, K., Naito, H., Arai, A., Kawakita, H., Aoki, W., 2016, ApJ, 818, 191

Uthas, H., Knigge, C., Steeghs, D., 2010, MNRAS, 409, 237

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Williams, R. & Mason, E., 2010, Ap&SS, 327, 207

Williams, R. 2013, AJ, 146, 55

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