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A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star- Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama Radio Observatory b Shizuoka Univ. c Sophia Univ. d ○M. Araki a , S. Takano b , H. Yamabe a , N. Koshikawa a , K. Tsukiyama a , A. Nakane c , T. Okabayashi c , A. Kunimatsu d , N. Kuze d

A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

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Page 1: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

A Search for the Interstellar Linear Carbon-Chain Alcohol HC4OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1

Tokyo Univ. of Sciencea Nobeyama Radio Observatoryb Shizuoka Univ.c Sophia Univ.d

○M. Arakia, S. Takanob, H. Yamabea, N. Koshikawaa, K. Tsukiyamaa, A. Nakanec, T. Okabayashic, A. Kunimatsud, N. Kuzed

Page 2: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

1. Introduction

HC4OH: Candidate of a New Interstellar Molecule 2007 Sophia Univ. Stark-Modulation MW Spectroscopy 2010 Shizuoka Univ. FT-MW Spectroscopy

Chemical Composition of Interstellar Space

Interstellar Molecules ~160 species

Linear Carbon Chain: 33 speciesAlcohol: MeOH, EtOH, Vinyl Alcohol

Linear Carbon-Chain Alcohol : New Category

→ Search for HC4OH

Page 3: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Low-mass star-forming region L1527

Dark cloud TMC-1

Target clouds• Rich carbon chains

2. Observations

• Rich O bearing molecules

Page 4: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Observed Molecules in L1527

Page 5: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

R.A.

(J2000)

Decl.

(J2000)

TMC-1 4h 41m 42.49s 25d 41' 27".0

L1527 4h 39m 53.89s 26d 03' 11".0

Outdoor sky map 2000

Galactic Plane

The equinoctial

Page 6: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Taurus Dark-Clouds Region

Galactic Longitude [degree]

Gal

actic

Lat

itude

[de

gree

]

Tokyo Gakugei University, http://darkclouds.u-gakugei.ac.jp/

TMC-1

L1527

Light Extinction

Page 7: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

TelescopeNobeyama Radio Observatory 45m Telescope

Date   2009/04/11-17 L1527, TMC-12010/01/15-21 L15272011/03/04-05 L1527

Integration Time 1~ 2 h

Search  Deepness Several mK in Antenna Temp.

Page 8: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Observed Transitions of HC4OH

S40H30H22

6K TMC-110K L1527

Ka = 0

High-Resolution Search

Page 9: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Observed Lines

C4H NJ = 45 – 34 38.1

NJ = 44 – 33 38.1

NJ = 910 – 89b 85.6

NJ = 99 – 88b 85.7

HC5N  J = 16 – 15 b 42.6

b Sakai et al. 2008, 2009a Kuze et al. in preparation.

GHz

HC4OHa JKa,Kc = 50,5 – 40,4 21.3

JKa,Kc = 70,7 – 60,6 29.8

JKa,Kc = 90,9 – 80,8 38.3

JKa,Kc = 100,10 – 90,9 42.5

JKa,Kc = 110,11–100,10 46.7

Page 10: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

TelescopeNobeyama Radio Observatory 45m Telescope

Date   2009/04/11-17 L1527, TMC-12010/01/15-21 L15272011/03/04-05 L1527

Integration Time 1~ 2 h

Search  Deepness Several mK in Antenna Temp.

Page 11: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

3. Results and Discussion

Page 12: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

VLSR(kms-1)

VLSR(kms-1)

TA

* (K

)

TMC-1

L1527

21.3

29.8

38.3

42.5

46.7

42.6 GHz

HC4OHNo Detection

Page 13: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

42.5

42.6 GHz

38.1

L1527

Page 14: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

NRO 45 m 38.9"

Integrated Intensity0.422 Kkms-1

33"0.585 Kkms-1

VLSR(kms-1)

TA

* (K

)

HC5N J = 16-1542.6 GHz

NRO

GBT 100 m 17.5" Sakai et al. 2009

Distribution of HC4OH in L1527

HC4CN (HC5N) = HC4OH

Page 15: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

L1527 TMC-1Column Density  

HC4OH < 2.0 1012 < 5.6 1012 cm-2

C4H 1.01 1014 2.9 1014 * cm-2

HC5N 6.8 1012 * 6.3 1013 ** cm-2

Excitation Temperature

HC4OH 12.3 fix(C4H2*) 3.8 fix(C4H2*) K

C4H 14.3 6.7 * K

HC5N 14.7* 6.5** K

Upper Limits of HC4OH Column Densities

(Local Thermal Equilibrium) * Sakai et al., 2008&2009, ** Takano et al. 1990

3 noise level

Page 16: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Column Density Ratios 

L1527 TMC-1

[HC4OH]/[HC5N] <0.3 <0.1

C4H 1 1

HC5N 1/15 1/5

HC4OH <1/52 <1/52

Page 17: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

What is a contribution to chemical reaction from the ratios?

No chemical reactions for HC4OH are reported.

Page 18: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Two schemes for Chemical Reactions of HC4OH

O/OH reacts with a carbon chain.OX(+) + C4X(+) XC4OX(+) HC4OH

O/OH extends a carbon chain.OX(+) XC2OX(+) XC4OX(+) HC4OH

The HC4OH/C4H ratio can contribute to know the chemical reactions of HC4OH.

Page 19: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

4. Summary

Upper limits of HC4OH < 2.0 1012 cm-2

HC5N > HC4OH

C4H >> HC4OH

Chemical Reactions of HC4OH

Deep Search of HC4OH

in L1527 and TMC-1

Page 20: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama
Page 21: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

C4H

Frequency 38.049617 GHz

NJ = 45-34

Frequency 38.088441 GHz

NJ = 44-33

Page 22: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

What is a contribution to chemical reaction from the ratios?

HC5N: Two Reaction Schemes

N/CN reacts with a carbon chain.CN extends a carbon chain.

No chemical reactions for HC4OH are reported.

Page 23: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

N/CN reacts with a carbon chain.

C+ + C4H → C5+ + H

C5+ + H2 → C5H+ + H

C5H+ + N → C5N+ + H

C5N+ + H2 → HC5N+ + H

HC5N+ + H2 → H2C5N+ + H

H2C5N+ + e → HC5N + H

HC4H + CN → HC5N + H

Millar & Freeman 1984

Fukuzawa & Osamura 1996

Page 24: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

CN extends a carbon chain.

HCNH+ + C2H2 → H2C2HCNH+ + h

H2C2HCNH+ + e- → HC2CN + H2

HC2CN + H3+ → HC2CNH+ + H2

H2C2CNH+ + C2H2 → H2C2 HC2CNH+ + H2

H2C2 HC2CNH+ + e- → HC4CN + H2 Mitchell et al. 1979

Page 25: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

Abundance ratios of C4H and HC5Nin Dark clouds

12

13

14

13 14 15

Log N(C4H)

Log

N(H

C5N

)

L1527

TMC-1

TMC-2

L1544

L183

L63B335

Millar & Freeman 1984

Page 26: A Search for the Interstellar Linear Carbon-Chain Alcohol HC 4 OH in the Star-Forming Region L1527 and the Dark Cloud TMC-1 Tokyo Univ. of Science a Nobeyama

What is a contribution to chemical reaction from the ratios?

HC5N: Two Reaction Schemes

N/CN reacts with a carbon chain.CN extends a carbon chain.

No chemical reactions for HC4OH are reported.