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From: Ali Al-Taani <ali82taani@yahoo.com>
Subject: LMXBs (Spin period and Orbital period)
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Date: Thu, 22 Apr 2010 02:42:17 -0700 (PDT)
From: Ali Al-Taani <ali82taani@yahoo.com>
Subject: LMXBs (Spin period and Orbital period)
To: xmmhelp@sciops.esa.int
--0-1414145358-1271929337=:23993
Content-Type: text/plain; charset=utf-8
Content-Transfer-Encoding: quoted-printable

Dear Team of XMM-Newton :=20
I=E2=80=99m Ali Taani from Jordan ; I=E2=80=99m PhD student in high energy =
astrophysics at National Astronomical Observatories which belong to Chinese=
 Academy of Science/Chian.=20
I writing you this email to ask you about the Table-Data for Low-Mass X-Ray=
 Binaries (LMXBs),=20
Actually, the data which I need LMXBs (Spin period and Orbital period),=C2=
=A0to make population synthesis for Millisecond Pulsars by using=20
Accretion Induced Collapse AIC.=20
So, it is a kind of you to help me to get these data=20
Looking forward to hearing from you=20
Sincerely=20
Ali Taani


Ali Al-Taani
Ph.D Student @ National Astronomical Observatories,
Chinese Academy of Sciences,
20A Datun Road ,
Chao yang District, Beijing 100012
China
Office:=C2=A0 +8664840732-1324
Mobile: +8618701432894
E-mail: alitaani@bao.ac.cn
=0A=0A=0A      
--0-1414145358-1271929337=:23993
Content-Type: text/html; charset=utf-8
Content-Transfer-Encoding: quoted-printable

<table cellspacing=3D"0" cellpadding=3D"0" border=3D"0" ><tr><td
valign=3D"=
top" style=3D"font: inherit;"><P style=3D"TEXT-ALIGN: left; MARGIN: 0in
0in=
 0pt; unicode-bidi: embed; DIRECTION: ltr" class=3DMsoNormal><FONT
size=3D3=
 face=3D"Times New Roman">Dear Team of XMM-Newton : </FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">I=E2=
=80=99m Ali Taani from <?xml:namespace prefix =3D st1 ns =3D "urn:schemas-m=
icrosoft-com:office:smarttags" /><st1:country-region
w:st=3D"on">Jordan</st=
1:country-region> ; I=E2=80=99m PhD student in high energy astrophysics at =
National Astronomical Observatories which belong to <st1:place
w:st=3D"on">=
<st1:PlaceName w:st=3D"on">Chinese</st1:PlaceName> <st1:PlaceType
w:st=3D"o=
n">Academy</st1:PlaceType></st1:place> of Science/Chian.
</FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">I wr=
iting you this email to ask you about the Table-Data for Low-Mass X-Ray Bin=
aries (LMXBs), </FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Actu=
ally, the data which I need LMXBs (<B><U>Spin period and Orbital
period</U>=
</B>),&nbsp;to make population synthesis for Millisecond Pulsars by
using <=
/FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Accr=
etion Induced Collapse AIC. </FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">So, =
it is a kind of you to help me to get these data </FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Look=
ing forward to hearing from you </FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Sinc=
erely </FONT></DIV>
<P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed; DIR=
ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Ali =
Taani</FONT></DIV><BR><BR><FONT color=3D#007f40
size=3D4 face=3D"bookman ol=
d style, new york, times, serif"><EM><EM><SPAN style=3D"COLOR:
#007f40; FON=
T-SIZE: 13.5pt">
<P style=3D"MARGIN: 0in 0in 0pt" class=3DMsoNormal><EM><SPAN
style=3D"COLOR=
: #007f40; FONT-SIZE: 13.5pt">Ali
Al-Taani</SPAN></EM></DIV>
<P style=3D"MARGIN: 0in 0in 0pt" class=3DMsoNormal><EM><SPAN
style=3D"COLOR=
: #007f40; FONT-SIZE: 13.5pt">Ph.D Student @ National Astronomical Observat=
ories,</SPAN></EM></DIV>
<P style=3D"MARGIN: 0in 0in 0pt" class=3DMsoNormal><EM><SPAN
style=3D"COLOR=
: #007f40; FONT-SIZE:
13.5pt">Chinese</SPAN></EM><EM><SPAN style=3D"COLOR: =
#007f40; FONT-SIZE: 13.5pt">
Academy</SPAN></EM><EM><SPAN style=3D"COLOR: #=
007f40; FONT-SIZE: 13.5pt"> of Sciences,</SPAN></EM></DIV>
<P style=3D"MARGIN: 0in 0in 0pt" class=3DMsoNormal><EM><SPAN
style=3D"COLOR=
: #007f40; FONT-SIZE: 13.5pt">20A Datun Road
,</SPAN></EM></DIV>
<P style=

Message of length 6311 truncated

Reply 1

Resend
From: Maria Diaz Trigo <xmmhelp@sciops.esa.int>
To: ali82taani@yahoo.com
Subject: Re: LMXBs (Spin period and Orbital period) (PR#43690)
Date: Thu Apr 22 10:29:25 2010
Dear Ali,

are you interested in tables related to XMM-Newton data, or to LMXBs in
general?
I would advise you to check the catalogue of LMXBs by Liu et al. 2007 at
http://adsabs.harvard.edu/abs/2007A%26A...469..807L. 

Best wishes,

Maria

Maria Diaz Trigo
XMM-Newton SOC

> --0-1414145358-1271929337=:23993
> Content-Type: text/plain; charset=utf-8
> Content-Transfer-Encoding: quoted-printable
> 
> Dear Team of XMM-Newton :=20
> I=E2=80=99m Ali Taani from Jordan ; I=E2=80=99m PhD student in high energy
=
> astrophysics at National Astronomical Observatories which belong to
Chinese=
>  Academy of Science/Chian.=20
> I writing you this email to ask you about the Table-Data for Low-Mass
X-Ray=
>  Binaries (LMXBs),=20
> Actually, the data which I need LMXBs (Spin period and Orbital
period),=C2=
> =A0to make population synthesis for Millisecond Pulsars by using=20
> Accretion Induced Collapse AIC.=20
> So, it is a kind of you to help me to get these data=20
> Looking forward to hearing from you=20
> Sincerely=20
> Ali Taani
> 
> 
> Ali Al-Taani
> Ph.D Student @ National Astronomical Observatories,
> Chinese Academy of Sciences,
> 20A Datun Road ,
> Chao yang District, Beijing 100012
> China
> Office:=C2=A0 +8664840732-1324
> Mobile: +8618701432894
> E-mail: alitaani@bao.ac.cn
> =0A=0A=0A      
> --0-1414145358-1271929337=:23993
> Content-Type: text/html; charset=utf-8
> Content-Transfer-Encoding: quoted-printable
> 
> <table cellspacing=3D"0" cellpadding=3D"0" border=3D"0"
><tr><td valign=3D"=
> top" style=3D"font: inherit;"><P style=3D"TEXT-ALIGN: left; MARGIN:
0in 0in=
>  0pt; unicode-bidi: embed; DIRECTION: ltr" class=3DMsoNormal><FONT
size=3D3=
>  face=3D"Times New Roman">Dear Team of XMM-Newton :
</FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">I=E2=
> =80=99m Ali Taani from <?xml:namespace prefix =3D st1 ns =3D
"urn:schemas-m=
> icrosoft-com:office:smarttags" /><st1:country-region
w:st=3D"on">Jordan</st=
> 1:country-region> ; I=E2=80=99m PhD student in high energy astrophysics
at =
> National Astronomical Observatories which belong to <st1:place
w:st=3D"on">=
> <st1:PlaceName w:st=3D"on">Chinese</st1:PlaceName>
<st1:PlaceType w:st=3D"o=
> n">Academy</st1:PlaceType></st1:place> of Science/Chian.
</FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">I wr=
> iting you this email to ask you about the Table-Data for Low-Mass X-Ray
Bin=
> aries (LMXBs), </FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Actu=
> ally, the data which I need LMXBs (<B><U>Spin period and
Orbital period</U>=
> </B>),.to make population synthesis for Millisecond Pulsars by using
<=
> /FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Accr=
> etion Induced Collapse AIC. </FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">So, =
> it is a kind of you to help me to get these data </FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Look=
> ing forward to hearing from you </FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Sinc=
> erely </FONT></DIV>
> <P style=3D"TEXT-ALIGN: left; MARGIN: 0in 0in 0pt; unicode-bidi: embed;
DIR=
> ECTION: ltr" class=3DMsoNormal><FONT size=3D3 face=3D"Times New
Roman">Ali =
> Taani</FONT></DIV><BR><BR><FONT color=3D#007f40
size=3D4 face=3D"bookman ol=
> d style, new york, times, serif"><EM><EM><SPAN
style=3D"COLOR: #007f40; FON=
> T-SIZE: 13.5pt">
> <P style=3D"MARGIN: 0in 0in 0pt" class=3DMsoNormal><EM><SPAN
style=3D"COLOR=
> : #007f40; FONT-SIZE: 13.5pt">Ali
Al-Taani</SPAN></EM></DIV>
> <P style=3D"MARGIN: 0in 0in 0pt" class=3DMsoNormal>&l

Message of length 7189 truncated

Up to top level
AO15   AO16   AO17   AO18   AO19   Backgrounds   Calibration   Conference   Data   Docs   EPICMOS   EPICpn   Feedback   Gallery   Misc   OM   Pending   PhD_Theses   Publications   RGS   RadMonitor   SAS_Hardware   SAS_WS   SASv16.0   SASv16.0_Installation   SASv16.1   SASv16.1_Installation   SASv17.0   SASv17.0_Installation   SASv18.0   SASv18.0_Installation   SciSim   Simulators_other   Suggestions   Trash   Visibility   XMM-bouncing   XMM-news   XRPS   XSA   esas   incoming  

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