G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See...

8
1 SUMMARY 1 G011.2-00.3 1 Summary Distance: 5 kpc ( Green et al., 1988 ) Position of Central Source (J2000): ( 18 11 29.2, -19 25 26.4 ) X-ray size: 4.5’x4.4’ Description: Circular outer shell with central source 1.1 Summary of Chandra Observations Sequence Obs ID Instrument Exposure uf Exposure f Date Observed Aimpoint (J2000) (ks) (ks) (α, δ) 500076 780 ACIS-235678 21.1 19.4 2000-08-06 ( 18 11 29.4, -19 25 25.0 ) Exposure uf Exposure time of un-filtered event file Exposure f Exposure time of filtered event file The whole remnant is covered by chip ACIS-S3(CCD ID=7) 1.2 Chandra Counts and Fluxes Region Energy Range Signal Rate F abs X F X L X (keV) (counts) (counts s 1 ) (ergs cm 2 s 1 ) (ergs cm 2 s 1 ) (ergs s 1 ) total 0.3 - 10.0 9.272e+04 4.791e+00 3.26e-11 3.98e-09 1.19e+37 ( 780 ) 0.3 - 2.1 7.100e+04 3.669e+00 1.47e-11 3.95e-09 1.18e+37 2.1 - 10. 2.202e+04 1.138e+00 1.80e-11 3.00e-11 8.94e+34 N H = 3.14 (10 22 cm 2 ) Assumed distance: 5 kpc ( Green et al., 1988 ) nH was derived with two thermal plasma model + power law 1 SUMMARY 2 1.3 Nearby Sources Obs ID Position (J2000) Size Net Count Count rate Note 780 ( 18 10 32.9, -19 17 53.3 ) 35.0” 114.0 5.40e-03 ( 18 10 49.2, -19 31 25.0 ) 16.3” 26.2 1.24e-03 ( 18 10 56.9, -19 34 00.7 ) 15.7” 63.4 3.00e-03 ( 18 10 59.6, -19 22 33.7 ) 8.7” 27.2 1.29e-03 ( 18 11 13.6, -19 33 42.0 ) 9.0” 267.0 1.26e-02 ( 18 11 17.1, -19 22 23.1 ) 5.9” 17.6 8.34e-04 ( 18 11 19.2, -19 26 33.1 ) 5.9” 97.2 4.60e-03 ( 18 11 19.3, -19 29 36.1 ) 5.9” 16.6 7.86e-04 ( 18 11 38.6, -19 24 26.0 ) 5.6” 59.3 2.81e-03 ( 18 11 40.6, -19 21 54.6 ) 4.6” 53.2 2.52e-03 ( 18 11 41.9, -19 28 15.4 ) 2.3” 41.3 1.96e-03 ( 18 11 42.1, -19 19 41.0 ) 8.8” 55.8 2.64e-03 ( 18 11 42.4, -19 18 42.9 ) 12.6” 25.9 1.23e-03 (note) 1. This nearby source list is incomplete. All the above sources are originally from the "src2.fits" file which is distributed with standard chandra processing. Only sources with significant count rate and which are clear to visual inspection are included. 2. The size given above is the size of the region used in detecting that source. 3. For each source, background was subtracted from annular region around the source. 1.4 References Green et al., 1988 MNRAS, 231, 735 : VLA at 1.4 and 5 GHz Vasisht et al., 1996 ApJ, 456L, 59 : ASCA

Transcript of G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See...

Page 1: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

1SU

MM

AR

Y1

G01

1.2-

00.3

1Su

mm

ary

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tanc

e:5

kpc

(G

reen

etal

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88)

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):(

1811

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5000

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who

lere

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bych

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and

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(G

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etal

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88)

nHw

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dw

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asm

am

odel

+po

wer

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2000

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ize

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ount

rate

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780

(18

1032

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)

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03

(note)

1.This

nearby

source

list

isincomplete.

All

the

above

sources

are

originally

from

the

"src2.fits"

file

which

isdistributed

with

standard

chandra

processing.

Only

sources

with

significant

count

rate

and

which

are

clear

tovisual

inspection

are

included.

2.The

size

given

above

isthe

size

ofthe

region

used

indetecting

that

source.

3.For

each

source,

background

was

subtracted

from

annular

region

around

the

source.

1.4

Ref

eren

ces

Gre

enet

al.,

1988

MN

RA

S,2

31,7

35:

VL

Aat

1.4

and

5G

Hz

Vas

isht

etal

.,19

96A

pJ,4

56L

,59

:A

SC

A

Page 2: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

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Page 3: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

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Page 4: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

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6

−1

9:2

5

−1

9:2

4

−1

9:2

3

RA (degree)

DEC (degree)

aci

s_E

12

20

−2

04

0_

S_

FL

UX

ED

.fits

_0

01

e−

06

2e

−0

63

e−

06

(counts/sec/cm^2)

18h11m18s

18h11m24s

18h11m30s

18h11m36s

−1

9:2

8

−1

9:2

7

−1

9:2

6

−1

9:2

5

−1

9:2

4

−1

9:2

3

RA (degree)

DEC (degree)

aci

s_E

20

40

−1

00

00

_S

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LU

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its_

0

01

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63

e−

06

(counts/sec/cm^2)

Page 5: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

5C

HA

ND

RA

SPE

CT

RU

M9

5C

hand

raSp

ectr

um

Imag

essh

owR

egio

nsus

edto

extr

acts

pect

ra

Reg

ions

with

red

stri

kes

are

excl

uded

5.1

Obs

ID78

0

Bac

kgro

und

was

subt

ract

edfr

omth

ere

gion

arou

ndth

eS

NR

.

tota

l

5C

HA

ND

RA

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CT

RU

M10

cent

rals

ourc

e

Page 6: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

5C

HA

ND

RA

SPE

CT

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M11

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AD

IOIM

AG

E12

6R

adio

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e

left

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dio

imag

e

righ

t:ch

andr

ax-

ray

imag

ew

ithra

dio

cont

our

lines

21-c

m -.Im

age

from

Gre

enet

al.(

1988

)-.

1G

Hz

flux

dens

ity:

22Jy

(cite

pGR

EE

N20

01)

18h11m18s

18h11m24s

18h11m30s

18h11m36s

−1

9:2

8

−1

9:2

7

−1

9:2

6

−1

9:2

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−1

9:2

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RA

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1.2

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cm_

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ge

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0

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0.004

0.006

0.008

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0.012

(mJy/Beam)

18h11m18s

18h11m24s

18h11m30s

18h11m36s

−1

9:2

8

−1

9:2

7

−1

9:2

6

−1

9:2

5

−1

9:2

4

−1

9:2

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RA (degree)

DEC (degree)

aci

s_E

30

0−

10

00

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FL

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(photons/cm^2/sec/pixel)

Sum

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Obs

erva

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scop

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VL

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Page 7: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

7IM

AG

ES

FRO

MSU

RV

EY

MIS

SIO

N13

7Im

ages

from

Surv

eyM

issi

on

Lef

t:C

hand

raIm

age

(0.3

-10.

keV

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Cen

ter

:Im

ages

from

SkyV

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with

asa

me

scal

e

righ

t:Im

ages

from

SkyV

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with

are

duce

dsc

ale

RO

SAT

PSP

C(1

.0de

g):

X-r

ay(0

.1-2

.4ke

V)

IRA

S12

mic

ron:

Infr

ared

(12

mic

ron)

IRA

S25

mic

ron:

Infr

ared

(25

mic

ron)

7IM

AG

ES

FRO

MSU

RV

EY

MIS

SIO

N14

IRA

S60

mic

ron:

Infr

ared

(60

mic

ron)

IRA

S10

0m

icro

n:In

frar

ed(1

00m

icro

n)

NR

AO

VL

ASk

ySu

rvey

(NV

SS):

Rad

io(1

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Hz

Con

tinu

um)

Page 8: G011.2-00.3 Summary - Harvard University · 2003. 8. 11. · 2 FIT DET AIL 3 2 Fit Detail See spectrum page for used re gions. 2.1 T otal: T w o thermal plsama model and po wer la

7IM

AG

ES

FRO

MSU

RV

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MIS

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Dig

itiz

edSk

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band

imag

esw

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afe

wex

cept

ions

)

The

Tw

oM

icro

nA

llSk

ySu

rvey

(J-b

and)

:IR

(1.2

5m

icro

ns)

The

Tw

oM

icro

nA

llSk

ySu

rvey

(H-b

and)

:IR

(1.6

5m

icro

ns)

7IM

AG

ES

FRO

MSU

RV

EY

MIS

SIO

N16

The

Tw

oM

icro

nA

llSk

ySu

rvey

(K-b

and)

:IR

(2.1

7m

icro

ns)