Estimated Thermal Emission from Bright Stars with Diameter > 10 mas

This table lists the estimated 100 GHz, 230 GHz, and 650 GHz thermal continuum fluxes from all stars with diameter larger than 10 milliarcsec listed in the paper by Ochsenbein & Halbwachs (1982, A&AS 47, 523-531). Effective temperature appropriate for the spectral type was taken from the Astrophysical Quantities by Allen (1973). [New additions are made based on Dyck et al. (1988, AJ 116, 981-986) on Sept. 9, 1998.]

Min S. Yun

National Radio Astronomy Observatory

August 5, 1998

 

Spect.

Diam.

100GHz

230GHz

650GHz

HD number

Name

RA B1950

Dec B1950

Vmag

Type

mas

mJy

mJy

mJy

124897

Alp Boo

14 13

+19 27

-0.04

K2 III

24.9

16

77

620

150798

Alp TrA

16 43

-68 56

1.92

K2 II

11.6

3.3

17

135

81797

Alp Hya

09 25

-08 26

1.98

K3 III

10.3

2.3

12

99

78647

Lam Vel

09 06

-43 14

2.21

K4 III

13.1

3.8

20

156

131873

Bet UMi

14 50

+74 22

2.08

K4 III

10.7

2.5

13

104

29139

Alp Tau

04 33

+16 25

0.85

K5 III

21.8

10

50

400

164058

Gam Dra

17 55

+51 30

2.24

K5 III

14.

4

21

164

6860

Bet And

01 07

+35 21

2.06

M0 III

12.0

2.8

15

121

148478

Alp Sco

16 26

-26 19

0.96

M1 II

45.7

38

190

1500

146051

Del Oph

16 12

-03 34

2.74

M1 III

26.

12

61

490

39801

Alp Ori

05 52

+07 24

0.50

M2 I

58.7

63

313

2500

206936

Mu Cep

21 42

+58 33

4.08

M2 I

20.4

7

36

290

18884

Alp Cet

02 59

+03 54

2.53

M2 III

16.

4.3

23

180

217906

Bet Peg

23 01

+27 49

2.42

M2 II-III

20.6

7.5

38

300

216386

Lam Aqr

22 50

-07 51

4.38

M2 I

13.3

2.8

15

123

44478

Mu Gem

06 20

+22 32

2.88

M3 III

14.

3.2

17

132

19058

Rho Per

03 02

+38 39

3.39

M3 III

19.

6.1

30

243

40239

Pi Aur

05 56

+45 56

4.26

M3 III

12.2

2.4

13

100

42995

Eta Gem

06 12

+22 31

3.28

M3 III

12.1

2.3

12

99

112300

Del Vir

12 53

+03 40

3.38

M3 III

11.6

2.2

11

91

108903

Gam Cru

12 28

-56 50

1.63

M4 III

41.1

28

140

1100

175589

Del2 Lyr

18 53

+36 50

4.30

M4 II

16.9

5

23

186

106849

Eps Mus

12 15

-67 41

4.11

M4 III

13.1

2.7

14

112

11695

Psi Phe

01 52

-46 33

4.41

M4 III

11.43

2.0

11

85

25705

Gam Ret

04 00

-62 18

4.51

M4 III

10.9

1.8

9.6

77

189763

62 Sgr

18 59

-27 51

4.58

M4 III

10.6

1.7

9.2

73

145366

Del1 Aps

16 13

-78 34

4.68

M4 III

10.3

1.6

8.6

70

214952

Bet Gru

22 39

-47 09

2.11

M5 III

52.2

43

210

1700

156014

Alp1 Her

17 12

+14 27

3.20

M5 III

37.1

22

110

860

175865

13 Lyr

18 54

+43 53

4.04

M5 III

21.

7.3

36

290

56096

LO2 Pup

07 12

-44 33

5.10

M5e

13.2

2.6

14

110

210967

Eps Oct

22 14

-80 41

5.10

M5 III

13.2

2.6

14

110

1760

T Cet

00 19

-20 20

5.12

M5 II

13.1

2.6

14

108

205730

W Cyg

21 34

+45 09

5.53

M5 III

11.4

2.4

13

102

113866

FS Com

13 04

+22 53

5.6

M5 III

10.5

1.6

8.6

69

14386

68Omi Cet

02 17

-03 12

3.04

M6 III

63.

60

300

2400

148783

30 Her

16 27

+41 59

5.04

M6 III

26.

10

51

410

189124

-

19 58

-59 31

5.17

M6 III

20.6

7

34

136

78712

-

09 08

+31 18

5.80

M6

15.1

3.2

17

136

18191

45Rho2Ari

02 53

+18 08

5.91

M6 III

14.4

3

16

125

163990

OB Her

17 55

+45 21

6.02

M6

13.7

2.7

14

113

109372

BO Mus

12 32

-67 29

6.1

M6 II-III

13.2

2.5

13

105

144205

X Her

16 02

+47 22

5.7

M7

12.2

2.7

14

114

108849

BK Vir

12 28

+04 41

7.46

M7 III

11.2

2.1

11

90

126327

RX Boo

14 22

+25 56

--

M7.5-8

18.8

5.7

30

240

29712

B Dor

04 36

-62 11

5.40

M8 III

45.7

29

150

1165

39816

U Ori

05 53

+20 10

5.40

M8 III

14.3

2.7

14

114

84748

R Leo

09 45

+11 40

6.02

M8 III

76?

80

400

3200