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		<id>https://en.formulasearchengine.com/w/index.php?title=Inverse_(mathematics)&amp;diff=11205</id>
		<title>Inverse (mathematics)</title>
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		<updated>2013-12-15T23:00:55Z</updated>

		<summary type="html">&lt;p&gt;71.116.229.228: Undid revision 586255593 by 71.116.229.228 (talk)&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{Starbox begin&lt;br /&gt;
 | name = 98 Aquarii&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox image&lt;br /&gt;
 | image = &lt;br /&gt;
     &amp;lt;div style=&amp;quot;position: relative&amp;quot;&amp;gt;[[File:Aquarius IAU.svg|250px|alt=Diagram showing star positions and boundaries of the Aquarius constellation and its surroundings]]&lt;br /&gt;
     &amp;lt;div style=&amp;quot;position: absolute; left: 27.6%; top: 57.6%&amp;quot;&amp;gt;[[File:Cercle rouge 100%.svg|12px]]&amp;lt;/div&amp;gt;&lt;br /&gt;
     &amp;lt;/div&amp;gt;&lt;br /&gt;
 | caption = Location of 98 Aquarii (circled)&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox observe&lt;br /&gt;
 | epoch       = J2000&lt;br /&gt;
 | ra          = {{RA|23|22|58.22606}}&amp;lt;ref name=aaa474_2_653/&amp;gt;&lt;br /&gt;
 | dec         = {{DEC|–20|06|02.0963}}&amp;lt;ref name=aaa474_2_653/&amp;gt;&lt;br /&gt;
 | appmag_v    = +3.97&amp;lt;ref name=mnras172_667/&amp;gt;&lt;br /&gt;
 | constell    = [[Aquarius (constellation)|Aquarius]]&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox character&lt;br /&gt;
 | class       = K0&amp;amp;nbsp;III&amp;lt;ref name=houk1978/&amp;gt;&lt;br /&gt;
 | b-v         = +1.089&amp;lt;ref name=mnras172_667/&amp;gt;&lt;br /&gt;
 | u-b         = +0.948&amp;lt;ref name=mnras172_667/&amp;gt;&lt;br /&gt;
 | variable    = &lt;br /&gt;
}}&lt;br /&gt;
{{Starbox astrometry&lt;br /&gt;
 | radial_v    = –6.5&amp;lt;ref name=scfs/&amp;gt;&lt;br /&gt;
 | prop_mo_ra  = –121.28&amp;lt;ref name=aaa474_2_653/&amp;gt;&lt;br /&gt;
 | prop_mo_dec = –97.59&amp;lt;ref name=aaa474_2_653/&amp;gt;&lt;br /&gt;
 | parallax    = 19.96&lt;br /&gt;
 | p_error     = 0.23&lt;br /&gt;
 | parallax_footnote = &amp;lt;ref name=aaa474_2_653/&amp;gt;&lt;br /&gt;
 | absmag_v    = &lt;br /&gt;
}}&lt;br /&gt;
{{Starbox detail&lt;br /&gt;
 | mass        = 2.1&amp;lt;ref name=aaa439_1_227/&amp;gt;&lt;br /&gt;
 | radius      = 14&amp;lt;ref name=lang2006/&amp;gt;&lt;br /&gt;
 | luminosity  = &lt;br /&gt;
 | gravity     = 2.4&amp;lt;ref name=aaa439_1_227/&amp;gt;&lt;br /&gt;
 | temperature = 4,630&amp;lt;ref name=aaa439_1_227/&amp;gt;&lt;br /&gt;
 | metal_fe    = –0.30&amp;lt;ref name=aaa439_1_227/&amp;gt;&lt;br /&gt;
 | rotational_velocity = &lt;br /&gt;
 | age_gyr     =&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox catalog&lt;br /&gt;
 | names= b&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&amp;amp;nbsp;Aquarii, [[Star catalogue#BD.2FCD.2FCPD|BD]]–20&amp;amp;nbsp;6587, [[FK5]]&amp;amp;nbsp;1612, [[Henry Draper Catalogue|HD]]&amp;amp;nbsp;220321, [[Hipparcos catalogue|HIP]]&amp;amp;nbsp;115438, [[Star catalogue#BS, BSC, HR|HR]]&amp;amp;nbsp;8892, [[Star catalogue#SAO|SAO]]&amp;amp;nbsp;191858.&amp;lt;ref name=SIMBAD/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox end}}&lt;br /&gt;
&#039;&#039;&#039;98 Aquarii&#039;&#039;&#039; is the [[Flamsteed designation]] for a [[star]] in the [[celestial equator|equatorial]] [[constellation]] [[Aquarius (constellation)|Aquarius]]. The [[Bayer designation]] for this star is b&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&amp;amp;nbsp;Aquarii. It is visible to the naked eye with an [[apparent visual magnitude]] of +3.97.&amp;lt;ref name=mnras172_667/&amp;gt; The distance to this star, {{Convert|163|ly|pc|abbr=off|lk=on}}, is known from [[parallax]] measurements made with the [[Hipparcos]] spacecraft.&amp;lt;ref name=aaa474_2_653/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
With over double the mass of the Sun,&amp;lt;ref name=aaa439_1_227/&amp;gt; this is an [[stellar evolution|evolved]] [[giant star]] that has a [[stellar classification]] of K0&amp;amp;nbsp;III.&amp;lt;ref name=houk1978/&amp;gt; The measured [[angular diameter]] of this star is {{nowrap|2.54 ± 0.13 [[milliarcsecond|mas]]}}.&amp;lt;ref name=aaa431_773/&amp;gt; At the estimated distance of 98 Aquarii,&amp;lt;ref name=aaa474_2_653/&amp;gt; this yields a physical size of about 14 times the [[Solar radius|radius of the Sun]].&amp;lt;ref name=lang2006/&amp;gt; The expanded outer envelope has an [[effective temperature]] of 4,630&amp;amp;nbsp;K,&amp;lt;ref name=aaa439_1_227/&amp;gt; giving it the orange glow of a [[K-type star]].&amp;lt;ref name=csiro/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist|refs=&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=aaa474_2_653&amp;gt;{{citation | first=F. | last=van Leeuwen |date=November 2007 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | bibcode=2007A&amp;amp;A...474..653V | doi=10.1051/0004-6361:20078357 | postscript=. |arxiv = 0708.1752 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=aaa439_1_227&amp;gt;{{citation | display-authors=1 | last1=Melo | first1=C. H. F. | last2=de Laverny | first2=P. | last3=Santos | first3=N. C. | last4=Israelian | first4=G. | last5=Randich | first5=S. | last6=Do Nascimento | first6=J. D., Jr. | last7=de Medeiros | first7=J. R. | title=On the nature of lithium-rich giant stars. Constraints from beryllium abundances | journal=Astronomy and Astrophysics | volume=439 | issue=1 | pages=227–235 |date=August 2005 | doi=10.1051/0004-6361:20041805 | bibcode=2005A&amp;amp;A...439..227M | arxiv=astro-ph/0504133 | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=houk1978&amp;gt;{{citation | last1=Houk | first1=Nancy | title=Michigan catalogue of two-dimensional spectral types for the HD stars | volume=4 | publication-place=Ann Arbor | publisher=Dept. of Astronomy, University of Michigan | year=1978 | bibcode=1988mcts.book.....H | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=scfs&amp;gt;{{citation | display-authors=1 | title=Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions | last1=Wielen | first1=R. | last2=Schwan | first2=H. | last3=Dettbarn | first3=C. | last4=Lenhardt | first4=H. | last5=Jahreiß | first5=H. | last6=Jährling | first6=R. | publisher=Astronomisches Rechen-Institut Heidelberg | issue=35 | year=1999 | bibcode=1999VeARI..35....1W | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=mnras172_667&amp;gt;{{citation | last1=Jennens | first1=P. A. | last2=Helfer | first2=H. L. | title=A new photometric metal abundance and luminosity calibration for field G and K giants. | journal=Monthly Notices of the Royal Astronomical Society | volume=172 | pages=667–679 |date=September 1975 | bibcode=1975MNRAS.172..667J | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=SIMBAD&amp;gt;{{citation | title=98 Aqr -- Star  | work=SIMBAD Astronomical Object Database | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=98+Aquarii | accessdate=2006-11-05 | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=aaa431_773&amp;gt;{{citation | last1=Richichi | pages=A. | last2=Percheron | first2=I. | last3=Khristoforova | first3=M. | title=CHARM2: An updated Catalog of High Angular Resolution Measurements | journal=Astronomy and Astrophysics | volume=431 | pages=773–777 |date=February 2005 | doi=10.1051/0004-6361:20042039 | bibcode=2005A&amp;amp;A...431..773R | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=lang2006&amp;gt;{{citation | first1=Kenneth R. | last1=Lang | title=Astrophysical formulae | volume=1 | series=Astronomy and astrophysics library | edition=3 | publisher=Birkhäuser | year=2006 | isbn=3-540-29692-1 | url=http://books.google.com/books?id=OvTjLcQ4MCQC&amp;amp;pg=PA41 | postscript=. }}. The radius (R&amp;lt;sub&amp;gt;*&amp;lt;/sub&amp;gt;) is given by:&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align} 2\cdot R_*&lt;br /&gt;
 &amp;amp; = \frac{(50.1\cdot 2.54\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\&lt;br /&gt;
 &amp;amp; \approx 27.4\cdot R_{\bigodot}&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=csiro&amp;gt;{{citation | title=The Colour of Stars | date=December 21, 2004 | work=Australia Telescope, Outreach and Education | publisher=Commonwealth Scientific and Industrial Research Organisation | url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html | accessdate=2012-01-16 | postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
{{Stars of Aquarius}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Flamsteed objects|Aquarii, 98]]&lt;br /&gt;
[[Category:Aquarius (constellation)]]&lt;br /&gt;
[[Category:K-type giants]]&lt;/div&gt;</summary>
		<author><name>71.116.229.228</name></author>
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		<title>Beta negative binomial distribution</title>
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		<updated>2012-06-25T22:11:44Z</updated>

		<summary type="html">&lt;p&gt;71.116.124.41: expressed PMF in Gamma function notation&lt;/p&gt;
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		<title>Schrödinger equation</title>
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		<updated>2008-03-17T05:02:09Z</updated>

		<summary type="html">&lt;p&gt;71.116.162.230: &lt;/p&gt;
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