_

separation indent medskip _language english _times 2 1 1 default

Title

Collapsed Cores in Globular Clusters, Gauge-Boson Couplings, and AASTeX atex

efault Examples Author

S. Djorgovski atex

altaffilmark<#8#>1,2,3<#8#> efault and Ivan R. King atex

altaffilmark<#9#>1<#9#> Affiliation

Astronomy Department, University of California, Berkeley, CA 94720 Author

C. D. Biemesderfer atex

altaffilmark<#10#>4,5<#10#> Affiliation

National Optical Astronomy Observatories, Tucson, AZ 85719 Email

aastex-help@aas.org And

Author

R. J. Hanisch atex

altaffilmark<#11#>5<#11#> Affiliation

Space Telescope Science Institute, Baltimore, MD 21218 Standard

atex

altaffiltext<#12#>1<#12#><#13#>Visiting Astronomer, Cerro Tololo Inter-American Observatory. CTIO is operated by AURA, Inc. under contract to the National Science Foundation.<#13#> Standard

atex

altaffiltext<#14#>2<#14#><#15#>Society of Fellows, Harvard University.<#15#> Standard

atex

altaffiltext<#16#>3<#16#><#17#>present address: Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138<#17#> Standard

atex

altaffiltext<#18#>4<#18#><#19#>Visiting Programmer, Space Telescope Science Institute<#19#>

Standard

atex

altaffiltext<#20#>5<#20#><#21#>Patron, Alonso's Bar and Grill<#21#> Abstract

This is a preliminary report on surface photometry of the major fraction of known globular clusters, to see which of them show the signs of a collapsed core. We also explore some diversionary mathematics and recreational tables.

Keywords

clusters: globular, peanut---bosons: bozos Section

Introduction Standard

A focal problem today in the dynamics of globular clusters is core collapse. It has been predicted by theory for decades atex

citep<#22#>hen61,lyn68,spi85<#22#> efault , but observation has been less alert to the phenomenon. For many years the central brightness peak in M15 atex

citep<#23#>kin75,new78<#23#> efault seemed a unique anomaly. Then atex

citet<#24#>aur82<#24#> efault suggested a central peak in NGC 6397, and a limited photographic survey of ours atex

citep[Paper I]<#25#>djo84<#25#> efault found three more cases, including NGC 6624, whose sharp center had often been remarked on atex

citep<#26#>can78<#26#> efault .

Section

Observations Standard

All our observations were short direct exposures with CCD's. At Lick Observatory we used a TI 500 _inset Formula × inset

500 chip and a GEC 575 _inset Formula × inset

385, on the 1-m Nickel reflector. The only filter available at Lick was red. At CTIO we used a GEC 575 _inset Formula × inset

385, with _inset Formula B, V, inset

and _inset Formula R inset

filters, and an RCA 512 _inset Formula × inset

320, with _inset Formula U, B, V, R, inset

and _inset Formula I inset

filters, on the 1.5-m reflector. In the CTIO observations we tried to concentrate on the shortest practicable wavelengths; but faintness, reddening, and poor short-wavelength sensitivity often kept us from observing in _inset Formula U inset

or even in _inset Formula B inset

. All four cameras had scales of the order of 0.4 arcsec/pixel, and our field sizes were around 3 arcmin. Standard

The CCD images are unfortunately not always suitable, for very poor clusters or for clusters with large cores. Since the latter are easily studied by other means, we augmented our own CCD profiles by collecting from the literature a number of star-count profiles

atex

citep<#27#>kin68,pet76,har84,ort85<#27#> efault , as well as photoelectric profiles atex

citep<#28#>kin66,kin75<#28#> efault and electronographic profiles atex

citep<#29#>kro84<#29#> efault . In a few cases we judged normality by eye estimates on one of the Sky Surveys. Section

Helicity Amplitudes Standard

It has been realized that helicity amplitudes provide a convenient means for Feynman diagram _float footnote Standard

Footnotes can be inserted like this. float evaluations. These amplitude-level techniques are particularly convenient for calculations involving many Feynman diagrams, where the usual trace techniques for the amplitude squared becomes unwieldy. Our calculations use the helicity techniques developed by other authors

_inset LatexCommand [#hag86##1###]

inset

; we briefly summarize below. Subsection

Formalism Standard

_inset LatexCommand

inset

Standard

A tree-level amplitude in _inset Formula #math7#e⁺e^- inset

collisions can be expressed in terms of fermion strings of the form _inset Formula

#math8#

#tex2html_wrap_indisplay865#(p₂, σ₂)P_-τ#tex2html_wrap_indisplay866##tex2html_wrap_indisplay867#^...#tex2html_wrap_indisplay868#u(p₁, σ₁),

(1)

inset

where _inset Formula p inset

and _inset Formula σ inset

label the initial _inset Formula e^± inset

four-momenta and helicities _inset Formula #math9#(σ = ±1) inset

, _inset Formula #math10##tex2html_wrap_inline874# = a^μ_iγ_ν inset

and _inset Formula #math11#P_τ = #tex2html_wrap_inline876#(1 + τγ₅) inset

is a chirality projection operator _inset Formula #math12#(τ = ±1) inset

. The _inset Formula #math13#a^μ_i inset

may be formed from particle four-momenta, gauge-boson polarization vectors or fermion strings with an uncontracted Lorentz index associated with final-sta te fermions. NoteToEditor

Figures 1 and 2 should appear side-by-side in print Standard

In the chiral representation the _inset Formula γ inset

matrices are expressed in terms of _inset Formula 2×2 inset

Pauli matrices _inset Formula σ inset

and the unit matrix 1 as _inset Formula

#math14#

γ^μ	=	#tex2html_wrap_indisplay886##tex2html_wrap_indisplay887##tex2html_wrap_indisplay888#, γ⁵ = #tex2html_wrap_indisplay889##tex2html_wrap_indisplay890##tex2html_wrap_indisplay891#,
σ^μ_±	=	(1,±σ),

inset

giving _inset Formula

#math15#

#tex2html_wrap_indisplay896# = #tex2html_wrap_indisplay897##tex2html_wrap_indisplay898##tex2html_wrap_indisplay899#,(#tex2html_wrap_indisplay900#)_± = a_μσ^μ_±,

(2)

inset

The spinors are expressed in terms of two-component Weyl spinors as _inset Formula

#math16#

u = #tex2html_wrap_indisplay902##tex2html_wrap_indisplay903##tex2html_wrap_indisplay904#, v = ((v)^†₊,(v)^†_-).

(3)

inset

Standard

The Weyl spinors are given in terms of helicity eigenstates _inset Formula #math17#χ_λ(p) inset

with _inset Formula #math18#λ = ±1 inset

by MathLetters

_inset Formula

#math19#

u(p, λ)_±	=	(E±λ\|p\|)^1/2χ_λ(p),	(4)
v(p, λ)_±	=	±λ(E#tex2html_wrap_indisplay914#λ\|p\|)^1/2χ_-λ(p)	(5)

inset

Section

Floating material and so forth Standard

Consider a task that computes profile parameters for a modified Lorentzian of the form _inset Formula

#math20#

I = #tex2html_wrap_indisplay916#

(6)

inset

where _inset Formula

#math21#

d₁ = #tex2html_wrap_indisplay918#

inset

_inset Formula

#math22#

d₂ = #tex2html_wrap_indisplay920#

inset

_inset Formula

#math23#

x₁ = (x - x₀)cosΘ + (y - y₀)sinΘ

inset

_inset Formula

#math24#

y₁ = - (x - x₀)sinΘ + (y - y₀)cosΘ

inset

Standard

In these expressions _inset Formula x₀ inset

, _inset Formula y₀ inset

is the star center, and _inset Formula Θ inset

is the angle with the _inset Formula x inset

axis. Results of this task are shown in table _separator

_inset LatexCommand #tbl-2#154>

inset

. It is not clear how these sorts of analyses may affect determination of

_inset Formula M_{#tex2html_wrap_inline928#} inset

, but the assumption is that the alternate results should be less than 90 atex

degr

efault out of phase with previous values. We have no observations of atex

ion<#156#>Ca<#156#><#157#>2<#157#> efault . Roughly atex

slantfrac<#158#>4<#158#><#159#>5<#159#> efault of the electronically submitted abstracts for AAS meetings are error-free. Acknowledgements

Standard

We are grateful to V. Barger, T. Han, and R. J. N. Phillips for doing the math in section _separator

_inset LatexCommand #bozomath#160>

inset

. More information on the AASTeX macros package are available at atex

_inset LatexCommand http://www.aas.org/publications/aastex

inset

efault or the atex

anchor<#162#>ftp://www.aas.org/pubs/<#162#><#163#>AAS ftp site<#163#> efault . Appendix

Section

Appendicial material Standard

Consider once again a task that computes profile parameters for a modified Lorentzian of the form _inset Formula

#math25#

I = #tex2html_wrap_indisplay930#

(7)

inset

where MathLetters

_inset Formula

#math26#

d₁ = #tex2html_wrap_indisplay932##tex2html_wrap_indisplay933#

inset

_inset Formula

#math27#

d₂ = #tex2html_wrap_indisplay935#34#tex2html_wrap_indisplay936#

(8)

inset

_inset Formula

#math28#

x₁	=	(x - x₀)cosΘ + (y - y₀)sinΘ	(9)
y₁	=	- (x - x₀)sinΘ + (y - y₀)cosΘ	(10)

inset

Standard

For completeness, here is one last equation.

_inset Formula

#math29#

e = mc²

(11)

inset

References

Aurière(1982)

Auriıè re, M. 1982, atex

aap efault , 109, 301 References

Canizares et al.(1978)

Canizares, C. R., Grindlay, J. E., Hiltner, W. A., Liller, W., and McClintock, J. E. 1978, atex

apj efault , 224, 39 References

Djorgovski and King(1984)

Djorgovski, S., and King, I. R. 1984, atex

apjl efault , 277, L49 References

Hagiwara and Zeppenfeld(1986)

Hagiwara, K., and Zeppenfeld, D. 1986, Nucl.Phys., 274, 1 References

Harris and van den Bergh(1984)

Harris, W. E., and van den Bergh, S. 1984, atex

aj efault , 89, 1816 References

Hènon(1961)

Hıé non, M. 1961, Ann.d'Ap., 24, 369 References

King(1966)

King, I. R. 1966, atex

aj efault , 71, 276 References

King(1975)

King, I. R. 1975, Dynamics of Stellar Systems, A. Hayli, Dordrecht: Reidel, 1975, 99 References

King et al.(1968)

King, I. R., Hedemann, E., Hodge, S. M., and White, R. E. 1968, atex

aj efault , 73, 456 References

Kron et al.(1984)

Kron, G. E., Hewitt, A. V., and Wasserman, L. H. 1984, atex

pasp efault , 96, 198 References

Lynden-Bell and Wood(1968)

Lynden-Bell, D., and Wood, R. 1968, atex

mnras efault , 138, 495 References

Newell and O'Neil(1978)

Newell, E. B., and O'Neil, E. J. 1978, atex

apjs efault , 37, 27 References

Ortolani et al.(1985)

Ortolani, S., Rosino, L., and Sandage, A. 1985, atex

aj efault , 90, 473 References

Peterson(1976)

Peterson, C. J. 1976, atex

aj efault , 81, 617 References

Spitzer(1985)

Spitzer, L. 1985, Dynamics of Star Clusters, J. Goodman and P. Hut, Dordrecht: Reidel, 109 Standard

atex

clearpage FigCaption

_inset LatexCommand

inset

This is the first figure and it uses sgi9259.eps as its EPS figure file. FigCaption

_inset LatexCommand

inset

This is an example of a long figure caption that must be set as a paragraph. The processor has to buffer the text of the caption, so it is good not to be too wordy, but that would make for poor communication as well.

FigCaption

_inset LatexCommand

inset

This figure has no associated EPS file, so the optional parameter is omitted.

Standard

atex

clearpage Standard

_float tab Caption _space_bottom medskip Terribly relevant tabular information. _inset LatexCommand

inset

Standard multicol5 7 13 0 0 -1 -1 -1 -1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 8 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 4 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 8 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 1 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 1 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 1 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 0 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 8 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot; 0 4 0 1 0 0 0 ;SPMquot;;SPMquot; ;SPMquot;;SPMquot;

Star
Height

_inset Formula d_x inset

_inset Formula d_y inset

_inset Formula n inset

_inset Formula χ² inset

_inset Formula R_maj inset

_inset Formula R_min inset

_inset Formula P inset

atex

tablenotemark<#238#>a<#238#> efault

_inset Formula PR_maj inset

_inset Formula PR_min inset

_inset Formula Θ inset

atex

tablenotemark<#241#>b<#241#> efault

Ref.

atex

tableline tableline efault 1
33472.5
-0.1
0.4
53
27.4
2.065
1.940
3.900
68.3
116.2
-27.639
1,2
2
27802.4
-0.3
-0.2
60
3.7
1.628
1.510
2.156
6.8
7.5
-26.764
3
3
29210.6
0.9
0.3
60
3.4
1.622
1.551
2.159
6.7
7.3
-40.272
4
4
32733.8
-1.2 atex

tablenotemark<#242#>c<#242#> efault

-0.5
41
54.8
2.282
2.156
4.313
117.4
78.2
-35.847
5,6
5
9607.4
-0.4
-0.4
60
1.4
1.669 atex

tablenotemark<#243#>c<#243#> efault

1.574
2.343
8.0
8.9
-33.417
7
6
31638.6
1.6
0.1
39
315.2
3.433
3.075
7.488
92.1
25.3
-12.052
8 Standard

atex

tablenotetext<#244#>a<#244#><#275#>Sample footnote for table~ ref<#245#>tbl-2<#245#> that was generated with the LaTeX table environment<#275#> Standard

atex

tablenotetext<#246#>b<#246#><#276#>Yet another sample footnote for table~ ref<#247#>tbl-2<#247#><#276#> Standard

atex

tablenotetext<#248#>c<#248#><#277#>Another sample footnote for table~ ref<#249#>tbl-2<#249#><#277#> TableComments

We can also attach a long-ish paragraph of explanatory material to a table. Use tablerefs to append a list of references. The following references were from a different table: I've patched them in here to show how they look, but don't take them too seriously---I certainly have not. TableRefs

(1) Barbuy, Spite, ;SPMamp; Spite 1985; (2) Bond 1980; (3) Carbon et al. 1987; (4) Hobbs ;SPMamp; Duncan 1987; (5) Gilroy et al. 1988: (6) Gratton ;SPMamp; Ortolani 1986; (7) Gratton ;SPMamp; Sneden 1987; (8) Gratton ;SPMamp; Sneden (1988); (9) Gratton ;SPMamp; Sneden 1991; (10) Kraft et al. 1982; (11) LCL, or Laird, 1990; (12) Leep ;SPMamp; Wallerstein 1981; (13) Luck ;SPMamp; Bond 1981; (14) Luck ;SPMamp; Bond 1985; (15) Magain 1987; (16) Magain 1989; (17) Peterson 1981; (18) Peterson, Kurucz, ;SPMamp; Carney 1990; (19) RMB; (20) Schuster ;SPMamp; Nissen 1988; (21) Schuster ;SPMamp; Nissen 1989b; (22) Spite et al. 1984; (23) Spite ;SPMamp; Spite 1986; (24) Hobbs ;SPMamp; Thorburn 1991; (25) Hobbs et al. 1991; (26) Olsen 1983. float Standard

atex To see this in action, uncomment the following Standard

atex efault

_inset Quotes eld inset

atex efault

_inset Quotes erd inset

atex ) and copy the file table.tex from the AASTeX 5.0 distribution into Standard

atex Standard

atex _inset Include 6 #center955#

inset

_end