A7IV MK73 dagger standard: iot UMa (=HR 3569) - A7IV Morgan71 standard: iot UMa (=HR 3569) - A7IV MorganAbt72 standard: iot UMa (=HR 3569) - A7IV Cowley74 standard: iot UMa (=HR 3569) - A7IV GarrisonGray89 standard: HR 3270 - A7IV [low-vsini stan.] iot UMa - A7IVn [high vsini stan.] The only two A7IV standards proposed appear to have HRD positions consistent with other dwarfs (both HR 3270 and iot UMa). Suggests that among late As, the spectral differences between dwarfs and subgiants are subtle and may not necessarily signify differences in luminosity. (B-V)(A7IV) = 0.237 ; (B-V)(A7V)=0.21 plus trend seen for other IV stars (B-V)(A7IV) = 0.233 ; exemplar kap Boo = HD 124675 (B-V)(A7IV) = 0.222 ; pri. stan. HD 70060 = HR 3270 (B-V)(A7IV) = 0.223(+-0.017 sem,+-0.036 stdev) ; SIMBAD median A7IV d<75pc,V<6.5(N=7) (B-V)(A7IV) = 0.223 ; deprecated stan. HD 76644 = iot UMa (B-V)(A7IV) = 0.191 ; exemplar gam Boo = HD 127762 => adopt (B-V)(A7IV) = 0.22 [updated 2/2/2022] Mv(A7IV) = 2.40 ; exemplar iot Boo = HR 5350 = HD 125161 (~main sequence) Mv(A7IV) = 2.31 ; exemplar HD 76644 = iot UMa (~main sequence) Mv(A7IV) = 2.16 ; pri. stan. HD 70060 = HR 3270 (~main sequence) Mv(A7IV) = 1.79(+-0.26 sem,+-0.59 stdev) ; SIMBAD median A7IV d<75pc,V<6.5(N=7) Mv(A7IV) = 1.5 ; GrayCorbally09 Mv(A7IV) = 1.05 ; exemplar kap Boo = HD 124675 Mv(A7IV) = 0.92 ; exemplar gam Boo = HD 127762 # No standards JM53 and Houk88 do not list a A7IV standard. # Primary Standard HD 70060 = HR 3270 (J0818-3639, V=4.4) *A7IV: GrayGarrison89(low-vsini stan.) A7III: Jaschek64(most),deVaucouleurs57, A4(M)A5-A7: Houk82 A5: Cannon A5/7: Loden69 Houk82 notes "HR 3270; |V SIN|I=130; OR COULD BE A5/7 III" Plx=34.93+-0.18 (HIP2), Vmag=4.44, B-V=0.222. HIP2 => Mv=2.16, and only 0.03 mag above main sequence! # Deprecated Standard HD 76644 = iot UMa = 9 UMa = HR 3569 = HIP 44127 A7V: JM53,Jaschek64(all),Cowley67,Cowley69(stan),Barry70,Gray03(A7Vn) *A7IV: MorganAbt72,MK73,Cowley74(stan),Garcia89,GrayGarrison89(high-vsini stan.) A6V: Palmer68 A5: Cannon V=3.12(HIP), B-V=0.223+-0.003(HIP), V-Ic=0.25(HIP). plx=68.92+-0.16mas(HIP2) => Mv=2.31 => 0.18 mag below MS, so seems to be MS. Spectroscopic binary. Basically A7V until ~Morgan72, then A7IV since until Gray03. M2V component "BC" only 3.7" away. # Exemplars gam Boo = HD 127762 = HR 5435 (J1432+3818; V=3.0) A7III: MK43,Cowley76(standard),Abt81 A7IIIn: Palmer68 *A7IV+(n): Gray01 A7IV+: GrayGarrison89 A7III-IV: Abt95 A5V: Adams35,Bouw81 Generally good agreement on "A7" temperature type due to use in MK43. However GrayGarrison89 and Gray01 consider the star to be "IV+" luminosity class. I've decided to list this star as a candidate "A7IV+" standard. (B-V)=0.191+-0.006(HIP). V=3.04(HIP). plx=37.58+-0.14mas(HIP2) => Mv=0.92 => 1.07 mag above MS. kap Boo = HD 124675 = HIP 69483 A6V+: GrayGarrison89 *A7IV: Slettebak55,Slettebak63,1962AnAp...25....1B,Palmer68,Gray01 A7V: Adams35,Abt81,Abt95 A8IV: Barry70(uv metals weak),Morgan72 A8V: Levato78 A9IV: 1958JO.....41..105B,Cowley69 F0V: Roman49 A of bright 14" cpm pair (STF 1821), with companion B (HIP 69481) of type F2V(Gray01) and Vmag=6.62. V=4.53(HIP), B-V=0.233+-0.012(HIP), V-I=0.23+-0.03(HIP). plx=20.1530+-0.0943mas(GaiaEDR3) => Mv=1.05 => 1.13 mag above MS. iot Boo = HR 5350 = HD 125161 = HIP 69713 A6V: Abt95 A7V: Slettebak55 *A7IV: Abt81,GrayGarrison89,Gray01(A7IV-) A8V: Barry70 A9V: Cowley69 37" binary. V=4.75(HIP), B-V=0.236+-0.015(HIP), V-I=0.19+-0.03(HIP). plx=33.8856+-0.082mas(GaiaEDR3) => Mv=2.40 => 0.20 mag below MS. # Other Stars JM53 lists Altair (alf Aql) and alf Cep as non-standard A7IV/V stars. Morgan65 classified only one Hyad as a subgiant: HD 28319 (= BD+15_632) as a A7IVn. But it is called A7III by MK78 and all subsequent literature (GrayGarrison89, Gray89, Gray01). HD 17093 = HR 812 = HIP 12832 A7III: Abt95 A7III-IV: Cowley69 *A7IV: 1951ApJ...113..304B,GrayGarrison89