28
INTERNATIONAL ASTRONOMICAL UNION SYMPOSIUM No. 95 PULSARS 13 Years of Research on Neutron Stars Edited by W. SIEBER and R. WIIEBINSKII D6 h INTERNATIONAL ASTRONOMICAL UNION D. REFDEL PUBLISHING COMPANY / DORDRECHT : HOLLAND ) BOSTTON:" O:SA. / LONDON: ENGLAND S p V! S/c-z tic VL' a,4? / IL __

SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 1: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

INTERNATIONAL ASTRONOMICAL UNION

SYMPOSIUM No. 95

PULSARS

13 Years of Research on Neutron Stars

Edited by W. SIEBER and R. WIIEBINSKII

D6 h

INTERNATIONAL ASTRONOMICAL UNION

D. REFDEL PUBLISHING COMPANY / DORDRECHT : HOLLAND )BOSTTON:" O:SA. / LONDON: ENGLAND

S p V! S/c-z tic VL' a,4? /

IL __

Page 2: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 3: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 4: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 5: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

o.

5630 Sawtelle BoulevardCulver City, California 90230April 29, 1968

M4isz S. Jocelyn Bell

ullard Radio Astronomy ObservatoryCambridge University, Ei gland

Dear Miss Beli:

I am writing to you about the unidentified radio emissions discovered by theastronomers at Cambridge University. These pulses have created great excitement

..... among scientists, and I would like to suggest a new theory about these pulses.

Sir Martin Ryle, head of Cambridge University' s Radio Astronomy Department, says rthat the pulses are the most exciting astronomical discovery of all time.

The period of silence between the pulses is exactly the same every time---1.3372795 seconds. During my research, I noticed that this figure could be

indicated as 13-37-27-95. The next step would be to multiply 13 x 37, with theresult of 431. Three sepexrate encyclopedia's list an original height of431 feet for the Great Pyramid (circa 2600 B. C.).

It is possible that the 1.337 has some special relationship to the engineering .design and site of the Great Pyramid. The balance of this 1.337 unit is 2795.

To my astonishment, i discovered that these figures appear in order in pi--the ratio of the diameter of a circle to the circumference.

3.11592,65339;79,23.46264383-2--7--9--5....

The Great " " . .. ..The Great Pyramid's height (481) and base-side (755) appears to show the appro 'mate

proportion: 1: 3.14159 :: 481 : 755 x 2.

I noticed that the units contain the logical pattern of 79-79, 32-32 and 38-33,with the center at 26.

... The English alphabet has 26 letters. Therefore, A equals 1, B equals 2, C equals

3, D equals 4--to Z equals the same 26.

A-B-C-D-E-G-G-H-I-J-K-L-M-N-0-P-Q-R-S-T-U-V--.-X-Y-Z (totals) 351. Rechecking,I discovered that 13 x 27 (1.3 37 27 95) equals the same 351.

It is my opinion that the radio pulses seem to have some special relationship to

pi and to the mathematical design and location of the Great Pyramid. The pulses

may be an attempt to direct our attention to the mathematical propertizs of the

Great Pyramid aid to the possible mathematical-engineering design of the Earth.

Kenneth Larson

VICTOAY Rii~hCn.7!• .f

I.

Page 6: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

ii

f

+

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Tr -15 :5903 3 329.54 1300"01

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A

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0031-07

0

0834.06

0809+74 1919+21 1237+25 0959-54 2303+30 2045-16 0525+21

90 ,

2-3 Integrated pue profiles for 45 pulsars, all .plotted on the same longitude scale i(a 90(

bar is given in the bottom of the figurct. These profiles were recorded at frequencies

between 4(0 and 650 MHz. and are arranged in order of increasing pulse .period.

457

At-

/czcc

Zx&

7:5 siec

•1/-3

0833-45 -29 1449,64 1929.+10 0950.8 1556-44

115 1-) 1933.16 0736-40 1642-0 5 1240-64 15 -52 16040

2021.51 2217.47 00450-18 2016.26 8318-04 174 3-28 1957-26

Pc

sc '...- e---"

Page 7: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

-90 0

FIGc 1. An equal-area projection of the distribution of the 330 known pulsars in galactic coordinates. The galactic center is in the middle of thefigure and longitude increases to the left.

1953 Astron. 1. 86(12), December 1981 0004-.6256/81/121953-2$500.90 @ 1981 Am. Astron. Soc. 1953

Page 8: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

\ . ' " "' r 'r " , - " ' dt. i. y • "t , , ." .

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Page 9: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

I. 1

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Page 10: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

120 180 240Long itude (degrees)

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Page 11: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

Psi!R

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Page 12: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 13: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 14: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 15: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 16: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 17: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 18: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 19: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

+ 900

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180' 120 0 ,300 240°

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7-5 Mean line=of§ight magnetic field components in the paths to pulsars. For fieldsgreater than 0.1 pG the area of the circle is proportional to the field strength (a circlerepresenting a 1pG field is shown in the lower right corner). A cross within a circlemeans the rotation measure is positive (field directed toward the observer). [FromManchester et al., 1977.]

XI,a 3tiR 'r

Page 20: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

S00

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FIGURE ic:. RADIAL VELOCITY CURVES

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Page 21: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 22: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

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Page 23: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

1 Ae c

Ass/-o e:

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Page 24: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

P&S if 41i

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Page 25: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

(I,

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Page 26: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

Intensity (Janskys) Linear (Percent) Position Angle

0

.N ,

,+'

Circular (Percent)

* 0

. r

r0

Ca.

Page 27: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

Intensity (Janskys) Linear (Percent) Position Angle

01tN VO

NN1

N

Circular (Frcent)

S o=

0 S

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1'

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Page 28: SYMPOSIUM No. 95 · o. 5630 Sawtelle Boulevard Culver City, California 90230 April 29, 1968 M4isz S. Jocelyn Bell ullard Radio Astronomy Observatory Cambridge University, Ei gland

Circular Polarization (v)(Jy)

(0A0J N)0 0 0

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