Psi9 Aurigae

{{Short description|Star in the constellation Auriga}}

{{DISPLAYTITLE:Psi9 Aurigae}}

{{for|other stars with a similar Bayer designation|Psi Aurigae{{!}}ψ Aurigae}}

{{Starbox begin

| name = Psi9 Aurigae

}}

{{Starbox image

| image=

{{Location mark

|image=Auriga constellation map.svg|alt=|float=center|width=260

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=ψ9 Aurigae

|x=116|y=228

}}

| caption = Location of ψ9 Aurigae (circled)

}}

{{Starbox observe

| epoch = J2000

| ra = {{RA|06|56|32.05797}}

| dec = {{DEC|+46|16|26.3957}}

| appmag_v = 5.75

| constell = Auriga

}}

{{Starbox character

| class = B8 IIIe

| r-i =

| v-r =

| b-v = −0.06

| u-b = −0.46

| variable =

}}

{{Starbox astrometry

| radial_v = −41.1{{±|2.9}}

| prop_mo_ra = −3.263

| prop_mo_dec = +5.040

| pm_footnote =

| parallax = 3.4481

| p_error = 0.0560

| parallax_footnote =

| absmag_v = −2.03

}}

{{Starbox detail

| mass = 2.4

| radius = 3.7

| luminosity = 868

| temperature = 9,573

| gravity = 2.71

| metal_fe = −0.55

| rotational_velocity = 235

| age_myr =

}}

{{Starbox catalog

| names = {{odlist | B=ψ9 Aur | BD=+46 1203 | HD=50658 | HIP=33377 | HR=2568 | SAO=41446 }}

}}

{{Starbox reference

|Simbad=psi09+Aur

}}

{{Starbox end}}

Psi9 Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ9 Aurigae, and abbreviated Psi9 Aur or ψ9 Aur. This star is dimly visible to the naked eye with an apparent visual magnitude of 5.75. Based upon an annual parallax shift of {{val|3.45|ul=mas}}, the distance to this star is approximately {{Convert|950|ly|pc|abbr=off|lk=on}}. It is drifting closer to the Sun with a radial velocity of −41 km/s. This is most likely (88.5% chance) a runaway star, having a peculiar velocity of 31.8{{±|14.6|12.4}} km/s.

The spectrum of Psi9 Aurigae matches a giant star with a stellar classification of B8 IIIe. The 'e' suffix indicates this is a Be star that shows emission lines of hydrogen in its spectrum. This is caused by a circumstellar shell of hot gas. The emission undergoes variability on a time scale of sixteen years. This star is spinning rapidly with a projected rotational velocity of 235 km/s. It has 2.4 times the mass of the Sun and 3.7 times the Sun's radius. ψ9 Aur is radiating 868 times the luminosity of the Sun from its photosphere at an effective temperature of 9,573 K.

References

{{reflist|refs=

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{{Cite XHIP

| 33377 | mode=cs2 | postscript=.}}

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{{citation | last=Crawford | first=D. L. | title=U, b, v, and Hβ Photometry for the Bright B8- and B9-TYPE Stars | journal=Astrophysical Journal | volume=137 | page=530 |date=February 1963 | doi=10.1086/147526 | bibcode=1963ApJ...137..530C | postscript=. | doi-access=free }}

{{cite simbad | title=* psi09 Aur | access-date=2012-08-23 | mode=cs2 | postscript=. }}

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{{citation | postscript=.

| title=On the kinematics of a runaway Be star population

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| journal=Monthly Notices of the Royal Astronomical Society

| volume=477 | issue=4 | pages=5261–5278 | date=July 2018

| doi=10.1093/mnras/sty980 | doi-access=free

| arxiv=1804.05849

| bibcode=2018MNRAS.477.5261B }}

}}