HD 25558
{{short description|Variable star in the constellation Taurus}}
{{Starbox begin}}
{{Starbox image
| image = 250px
| caption = A light curve for V1133 Tauri, plotted from TESS data. The 1.53 day period is marked in red.
}}
{{Starbox observe
| epoch = J2000.0
| dec = {{DEC|+05|26|08.2258}}
| constell = Taurus
}}
{{Starbox character
| b-v =
| u-b =
| variable = Slowly pulsating B-type star
}}
{{Starbox astrometry
| radial_v =
| prop_mo_ra = {{val|1.271|0.275}}
| prop_mo_dec = {{val|-7.216|0.201}}
| parallax = 4.5161
| p_error = 0.2637
}}
{{Starbox detail
| component1 = Primary
| mass = 4.6
| radius = 2.4{{efn|name=radius}}
| luminosity = {{val|560|530|270}}
| temperature = {{val|fmt=commas|16850|800}}
| metal_fe = −0.3
| gravity = {{val|4.2|0.2}}
| rotational_velocity = {{val|21.5|1.5}}
| rotation = {{val|5.9|2|ul=days}}
| age_gyr =
| component2 = Secondary
| mass2 = 4.2
| radius2 = 2.9{{efn|name=radius}}
| luminosity2 = {{val|420|540|230}}
| temperature2 = {{val|fmt=commas|16250|1000}}
| gravity2 = {{val|4.25|0.25}}
| rotational_velocity2 = {{val|35|4}}
| rotation2 = {{val|1.2|0.6|ul=days}}
| metal_fe2 = −0.3
| age_myr2 = 40-55
}}
{{Starbox catalog
| names = 40 Tauri, V1133 Tau, BD+05 584, HIP 18957, HR 1253, SAO 111585
}}
{{Starbox reference
| Simbad = 40+Tau
}}
{{Starbox end}}
HD 25558, also known as V1133 Tauri and by its Flamsteed designation 40 Tauri, is a star located about 700 light years from the Earth, in the constellation Taurus. Its apparent magnitude is about 5.3, making it faintly visible to the naked eye of an observer far from city lights. It is a variable star, ranging in brightness from Hipparcos magnitude 5.28 to 5.32 over a period of 1.53232423 days.
In 1998, HD 25558 was discovered to be a variable star by Christoffel Waelkens et al. who analyzed the Hipparcos photometric data for hundreds of stars, and classified HD 25558 as a slowly pulsating B star with a period of 1.53 days.
Beginning in 2008, HD 25558 was the subject of an observing campaign by Ádám Sódor et al. who gathered data collected from 17 observatories on the ground and in space. This star was chosen for the project because it is relatively bright, located near the celestial equator (and thus observable from almost anywhere on Earth), and the slow rotation indicated in earlier studies would simplify the interpretation of spectra. The investigators concluded that HD 25558 is a spectroscopic binary with a period of about 8.9 years, but not enough data was available to derive a full description of the orbit. Both components of the binary show detectable stellar pulsations. The primary star rotates with a period of about 6 days, and the secondary rotates in just 1.2 days. The primary has no detectable magnetic field, but the secondary's field strength is at least a few hundred gauss. The dominant 1.53 day pulsation period arises from the primary star and those pulsations were coherent over the 20 year period spanned by the data used in the study.
Notes
{{notelist|refs=
{{efn|name=radius|The paper derives the period from the rotational velocity and the radius, but does not show the radius. The radius found can be calculated from the period and equatorial rotational velocity.}}
}}
References
{{Reflist|30em|refs=
| title=The magnetic early B-type Stars II: stellar atmospheric parameters in the era of Gaia
| last1=Shultz | first1=M. E. | last2=Wade | first2=G. A.
| last3=Rivinius | first3=Th | last4=Alecian | first4=E.
| last5=Neiner | first5=C. | last6=Petit | first6=V.
| last7=Wisniewski | first7=J. P. | last8=BinaMIcS Collaboration
| display-authors=1 | journal=Monthly Notices of the Royal Astronomical Society
| volume=485 | issue=2 | pages=1508–1527 | date=May 2019
| doi=10.1093/mnras/stz416 | doi-access=free | arxiv=1902.02713
| bibcode=2019MNRAS.485.1508S }}
| title=MAST: Barbara A. Mikulski Archive for Space Telescopes
| url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html
| publisher=Space Telescope Science Institute |access-date=16 January 2023}}
{{cite Gaia DR3|3272902041766301184}}
| last1=Ducati | first1=J. R.
| title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system
| url=https://cdsarc.cds.unistra.fr/viz-bin/cat/II/237#/browse
| journal=Vizier Online Data Catalog | year=2002
| volume=2237
| bibcode=2002yCat.2237....0D
| publisher=Strasbourg astronomical Data Center | access-date=17 January 2023}}
| title=V1133 Tau | url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=36150
| website=International Variable Star Index
| publisher=AAVSO | access-date=17 January 2023}}
| title=40 Tau -- Double or Multiple Star | access-date=2023-01-16}}
| last1=Waelkens | first1=C. | last2=Aerts | first2=C.
| last3=Kestens | first3=E. |last4=Grenon | first4=M. | last5=Eyer | first5=L.
| title=Study of an unbiased sample of B stars observed with Hipparcos: the discovery of a large amount of new slowly pulsating B stars
| journal=Astronomy and Astrophysics | date=February 1998 | volume=330 | pages=215–221 | bibcode=1998A&A...330..215W }}
{{cite journal | last1=Sódor | first1=Á. | last2=De Cat | first2=P. | last3=Wright | first3=D. J.
| last4=Neiner | first4=C. | last5=Briquet | first5=M. | last6=Lampens | first6=P. | last7=Dukes | first7=R. J.
| last8=Henry | first8=G. W. | last9=Williamson | first9=M. H. | last10=Brunsden | first10=E. | last11=Pollard | first11=K. R.
| last12=Cottrell | first12=P. L. | last13=Maisonneuve | first13=F. | last14=Kilmartin | first14=P. M.
| last15=Matthews | first15=J. | last16=Kallinger | first16=T. |last17=Beck | first17=P. G. | last18=Kambe | first18=E.
| last19=Engelbrecht | first19=C. A. | last20=Czanik | first20=R. J. | last21=Yang | first21=S.
| last22=Hashimoto | first22=O. | last23=Honda | first23=S. | last24=Fu | first24=J. N.
| last25=Castanheira | first25=B. | last26=Lehmann | first26=H. | last27=Bognár | first27=Zs. | last28=Behara
| first28=N. | last29=Scaringi | first29=S. | last30=Van Winckel | first30=H. | last31=Menu | first31=J.
| last32=Lobel | first32=A. | last33=Mathias | first33=P. | last34=Saesen | first34=S. | last35=Vučković
| first35=M. | last36=the MiMeS collaboration
| title=Extensive study of HD 25558, a long-period double-lined binary with two SPB components
| journal=Monthly Notices of the Royal Astronomical Society
| date=March 2014 | volume=438 | issue=4 | pages=3535–3556
| doi=10.1093/mnras/stt2466 | arxiv=1312.6307 | bibcode=2014MNRAS.438.3535S | doi-access=free }}
}}
{{Stars of Taurus}}
{{DEFAULTSORT:HD 25558}}
Category:Slowly pulsating B-type stars
Category:Taurus (constellation)