Root-mean-square deviation: Difference between revisions

From formulasearchengine
Jump to navigation Jump to search
en>Rjwilmsi
m Journal cites, using AWB (9871)
en>Fernando.iglesiasg
Formula: The regression's dependent variable should not have time sub-index.
 
(One intermediate revision by one other user not shown)
Line 1: Line 1:
{{Starbox begin
Hi there. My title is Sophia Meagher even though it is not the name on my birth certification. My working day occupation is an invoicing officer but I've already utilized for another one. For many years she's been residing in Kentucky but her spouse wants them to transfer. What I adore doing is soccer but I don't have the time recently.<br><br>Feel free to surf to my  [http://brazil.amor-amore.com/irboothe certified psychics] homepage: free [http://appin.co.kr/board_Zqtv22/688025 good psychic] readings ([http://cpacs.org/index.php?document_srl=90091&mid=board_zTGg26 Privacy of Data: This tool is built-with and functions-in Client Side JavaScripting, so only your computer will see or process your data input/output.a cool way to improve])
| name = HR 3803
}}
{{Starbox observe
| epoch    = J2000
| constell = [[Vela (constellation)|Vela]]
| ra      = {{RA|09|31|13.31891}}<ref name=aaa474_2_653/>
| dec      = {{DEC|–57|02|03.7578}}<ref name=aaa474_2_653/>
| appmag_v = 3.16<ref name=scfs/>
}}
{{Starbox character
| class    = K5&nbsp;III<ref name=araa11_29/>
| b-v      = +1.55<ref name=clpl4_99/>
| u-b      = +1.88<ref name=clpl4_99/>
| variable =
}}
{{Starbox astrometry
| radial_v = –13.9<ref name=scfs/>
| prop_mo_ra  = –32.54<ref name=aaa474_2_653/>
| prop_mo_dec = +5.87<ref name=aaa474_2_653/>
| parallax = 13.65
| p_error  = 0.10
| parallax_footnote = <ref name=aaa474_2_653/>
| absmag_v =
}}
{{Starbox detail
| mass    = 2.0<ref name=aaa352_217/>
| radius  = 29<ref name=lang2006/>
| luminosity  =
| temperature = 3,860<ref name=aaa352_217/>
| gravity  =
| metal_fe =
| rotational_velocity =
}}
{{Starbox catalog
| names = [[Bayer designation|N]] Velorum, N Vel, [[Star catalogue#BD.2FCD.2FCPD|CP]]–56&nbsp;2270, [[Henry Draper Catalogue|HD]]&nbsp;82668, [[Catalogues of Fundamental Stars|FK5]]&nbsp;361, [[Hipparcos catalogue|HIP]]&nbsp;46701, [[Star catalogue#BS, BSC, HR|HR]]&nbsp;3803, [[Star catalogue#SAO|SAO]]&nbsp;237067.
}}
{{Starbox end}}
'''HR 3803''' or '''N Velorum''' (N Vel) is a 3rd-[[Apparent magnitude|magnitude]] [[star]] on the border between the southern [[constellation]]s [[Carina (constellation)|Carina]] and [[Vela (constellation)|Vela]]. Based upon [[parallax]] measurements, it is approximately {{Convert|239|ly|pc|abbr=off|lk=on}} from [[Earth]]. It is an orange-hued [[stellar classification|K-type]] [[giant star]] and has twice the mass of the Sun.<ref name=aaa352_217/> The measured [[angular diameter]] of this star, after correction for [[limb darkening]], is {{nowrap|7.13 ± 0.08 [[milliarcsecond|mas]]}}.<ref name=aaa431_773/> At the estimated distance of Eta Draconis,<ref name=aaa474_2_653/> this yields a physical size of about 29 times the [[Solar radius|radius of the Sun]].<ref name=lang2006/>
 
In 1752, French astronomer [[Nicolas Louis de Lacaille]] divided the former constellation [[Argo Navis]] into three separate constellations, and then referenced its stars by extending [[Bayer designation|Bayer's system of star nomenclature]];<ref>http://homepage.mac.com/andjames/Page206.htm</ref> this star was given the designation ''N Velorum''. In 1871 [[Benjamin Apthorp Gould]] discovered this star to be [[variable star|variable]], but this occurred prior to the standardization of variable star nomenclature by German astronomer [[Friedrich Wilhelm Argelander]] during the nineteenth century, so it does not fall into the standard range of variable star designations.<ref name=jaavso16_2_65/>
 
The star should not be confused with [[HD 74272|n Velorum]].
 
==References==
{{reflist|refs=
 
<ref name=aaa474_2_653>{{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&A...474..653V | doi=10.1051/0004-6361:20078357 |arxiv = 0708.1752 }}</ref>
 
<ref name=aaa352_217>{{citation | last1=Gondoin | first1=P. | title=Evolution of X-ray activity and rotation on G-K giants | journal=Astronomy and Astrophysics | volume=352 | pages=217–227 |date=December 1999 | bibcode=1999A&A...352..217G }}</ref>
 
<ref name=araa11_29>{{cite journal | last1=Morgan | first1=W. W. | last2=Keenan | first2=P. C. | title=Spectral Classification | journal=Annual Review of Astronomy and Astrophysics | volume=11 | issue=1 | page=29 | year=1973 | doi=10.1146/annurev.aa.11.090173.000333 | bibcode=1973ARA&A..11...29M }}</ref>
 
<ref name=scfs>{{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 }}</ref>
 
<ref name=clpl4_99>{{cite journal | display-authors=1 | last1=Johnson | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966 | bibcode=1966CoLPL...4...99J }}</ref>
 
<ref name=jaavso16_2_65>{{citation | last1=Hoffleit | first1=Dorrit | title=History of Variable Star Nomenclature | journal=The Journal of the American Association of Variable Star Observers | volume=16 | issue=2 | pages=65–70 |date=December 1987 | bibcode=1987JAVSO..16...65H | url=http://www.aavso.org/files/webpublications/ejaavso/v16n2/65.pdf | accessdate=2012-02-02 }}</ref>
 
<ref name=aaa431_773>{{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&A...431..773R }}</ref>
 
<ref name=lang2006>{{citation | first1=Kenneth R. | last1=Lang | title=Astrophysical formulae | volume=1 | series=Astronomy and astrophysics library | edition=3 | publisher=Birkhäuser | year=2006 | isbn=3540296921 | url=http://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 }}. The radius (R<sub>*</sub>) is given by:
:<math>\begin{align} 2\cdot R_*
& = \frac{(73.3\cdot 3.72\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\
& \approx 58.7\cdot R_{\bigodot}
\end{align}</math></ref>
 
}}
{{Stars of Vela}}
 
{{DEFAULTSORT:Hd 82668}}
[[Category:Bayer objects|Velorum, N]]
[[Category:Henry Draper Catalogue objects|082668]]
[[Category:K-type giants]]
[[Category:Vela (constellation)]]
 
{{Giant-star-stub}}

Latest revision as of 11:57, 15 December 2014

Hi there. My title is Sophia Meagher even though it is not the name on my birth certification. My working day occupation is an invoicing officer but I've already utilized for another one. For many years she's been residing in Kentucky but her spouse wants them to transfer. What I adore doing is soccer but I don't have the time recently.

Feel free to surf to my certified psychics homepage: free good psychic readings (Privacy of Data: This tool is built-with and functions-in Client Side JavaScripting, so only your computer will see or process your data input/output.a cool way to improve)