Search results

| variable = [[Lambda Eridani variable|λ Eri]]<ref name=mnras277_4_1547/> It is a [[λ Eridani variable]], or [[periodic Be star]], with a pulsation cycle lasting 1.073 d ...

...riable = [[Gamma Cassiopeiae variable|GCAS]]<ref name=gcvs/> + [[Lambda Eridani variable|LERI]] ...Index lists Eta Centauri as both a Gamma Cassiopeiae variable and a Lambda Eridani variable with variations caused by its rotation and pulsations.<ref name=vs ...

'''Beta Cephei variables''', also known as '''Beta Canis Majoris stars''', are [[variable stars]] th Beta Cephei variables are somewhat [[stellar evolution|evolved]] stars of masses between about 7 ...

| title=Intensive photometry of southern Be variables. I. Winter objects [[Category:Lambda Eridani variables]] ...

...e up of a singular star. ''Xuange'', the [[halberd]], was represented by [[Lambda Boötis]], and ''Zhaoyao'', either the [[sword]] or the spear, was represent ...es]] and as subjects to study [[asteroseismology]].{{sfn|AAVSO Delta Scuti Variables}} ...

| data-sort-value="Eri α" |α [[Eridanus (constellation)|Eridani]] | [[Lambda Velorum|Suhail]] ...

...ry 2001 |title=The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. II. Results from 12&nbsp;galactic cluster ...ay 2000 |title=The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. I. Results from 19&nbsp;OB&nbsp;associati ...

...May 2000|title=The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. I. Results from 19 OB Associations in the ...ate=2019-09-01 |title=On the Gaia DR2 distances for Galactic luminous blue variables |journal=Monthly Notices of the Royal Astronomical Society |volume=488 |iss ...