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=== 100–700 solar radii === |
=== 100–700 solar radii === |
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Revision as of 12:30, 25 June 2024
This is the 6th list of the "stars by size" lists.
List
Legend
Bright star (Mv ≤ 3.5m) |
100–700 solar radii
Name | Radius
(R☉) |
Constellation | Sp. type | Note | |
---|---|---|---|---|---|
S Doradus | 100 – 380[1] | Dorado | Be3 C[2] | ||
30 Piscium | 100.17+2.67 −3.81[3] |
Pisces | M3III[3] | ||
Tau4 Eridani | 102.9[4] | Eridanus | M3.5III[4] | ||
Scheat | 104[5][a] | Pegasus | M2.5II-III[6] | 84th brightest star in the night sky | |
Sigma Ophiuchi | 106 – 109[7] | Ophiuchus | K2II[8] | ||
Tejat | 107.7[4] | Gemini | M3IIIab B[9] | ||
Sigma Librae | 109[5][a] | Libra | M2.5III[5] | ||
Zeta1 Scorpii | 112.4[10] | Scorpius | B1.5Ia+[10] | A blue hypergiant. | |
RR Ursae Minoris | 113.9+5.4 −6[3] |
Ursa Minor | M4III[3] | ||
Zeta Arae | 114±4[11] | Ara | K3III[11] | ||
V378 Normae | 115[12] | Norma | G8Ib[13] | ||
Epsilon Muscae | 116±9[14] | Musca | M4III[15] | ||
AW Canum Venaticorum A | 117.41+4.25 −4.57[16] |
Canes Venatici | M3III[16] | ||
3 Aquarii | 117.6+4 −4.2[3] |
Aquarius | M3III[3] | ||
Hassaleh | 123.8;[17][b] 151[18][c] | Auriga | K3II-III[19] | ||
V337 Carinae | 128±12[14] | Carina | K2.5II[20] | ||
34 Boötis | 129.36+7.49 −8.42[16] |
Boötes | M3III[16] | ||
Mebsuta | 130.22+5.51 −6.01[16]; 123 – 168[21][d] |
Gemini | G8 I[16] | ||
HD 268835 (R126) | 130.88[22] | Mensa | B8Ia[22] | Blue hypergiant surrounded by a massive dust disk | |
TV Piscium | 136[23] | Pisces | M3III[23] | ||
Tiaki | 137.6[23] | Grus | M4.5III[24] | 62nd brightest star in the night sky | |
GZ Velorum | 141±11[14] | Vela | K2.5II[25] | ||
Rho Persei | 143[14]–157.3[5][a] | Perseus | M4IIIa[26] | ||
Epsilon Aurigae | 143 – 358[27] | Auriga | F0I[28] – A9Ia[29] | Erroneously considered as the largest known star, with a radius of 2,700 to 3,000 R☉. | |
Atria | 143.5[30] | Triangulum Australe | K2III_Ba1 C[31] | 42rd brightest star in the night sky | |
L2 Puppis | 145.21[32] | Puppis | M5IIIe[33] | ||
HD 210762 | 151.06 – 181.32[7] | Pegasus | K0[34] | ||
Omega Capricorni | 167.39[7] | Capricornus | M0IIIBa0.5[35] | ||
l Carinae | 169±8[36] | Carina | G5Iab/b[37] | ||
Zeta Cephei | 172.7+7.5 −8.3[3] |
Cepheus | K1.5Ib[38] | ||
Eta Persei | 173.1+9.69 −10.8[39] |
Perseus | K3I-II | ||
Gamma Cygni | 174[e] | Cygnus | F8Ib[40] | ||
Omicron2 Cygni | 183.2+10.1 −11.35[3] |
Cygnus | K1III[3] | ||
30 Herculis | 188[5][a] | Hercules | M6III[41] | ||
R Lyrae (13 Lyrae) | 195.08[5][a] | Lyra | M4.5III[42] | ||
72 Leonis | 195.4+31.4 −46.2[16] |
Leo | M3IIb:[43] | ||
24 Sagittarii | 197.3[7] | Sagittarius | K3III C[44] | ||
OP Herculis | 202.8[5][a] | Hercules | M6S[45] | ||
Deneb | 203±17[46] | Cygnus | A2Ia C[47] | 19th brightest star in the night sky. Prototype of the Alpha Cygni variables. | |
Suhail | 210[48] | Vela | K5Ib[48] | 65th brightest star in the night sky | |
Enif (epsilon Pegasi) | 210.37 – 210.69[7] | Pegasus | K2Ib-II[49] | ||
NS Puppis | 213±24[14] | Puppis | K4.5Ib[50] | ||
S Crateris | 213.3[32] | Crater | M6III[51] | ||
Omicrion1 Orionis | 214±29[11] | Orion | M3S III[52] | ||
Wezen | 215±66; 194.6–204.4 [f][53] | Canis Major | F8Ia[54] | 36th brightest star in the night sky | |
NP Puppis | 219[55] | Puppis? | C-N4.5[56] | ||
Xi Cygni | 220.09+9.64 −10.56[3] |
Cygnus | K4.5Ib-II[57] | ||
W Cygni | 227[32] | Cygnus | M4IIIe–M6IIIe[58] | ||
Y Pavonis | 228[55] | Pavo? | C | ||
V420 Vulpeculae | 234.1[23] | Vulpecula | N:e:[23] | ||
BG Cygni | 236±76[59] | Cygnus | M8e[60] | ||
RX Boötis | 237.1[32] | Boötes | M7.5-M8[61] | ||
R Doradus | 240[23] – 298±21[62] | Dorado | M8III:e[23] | Largest star in terms of angular diameter | |
Eta Carinae A | 240[63] | Carina | LBV[64] | One of the most massive known stars. A luminous blue variable. | |
R Carinae | 241[32] | Carina | M5-M8[65] | ||
SW Virginis | 244±42[66] | Virgo | M7III:[67] | ||
70 Sagittarii (BS6861) | 250[5][a] | Sagittarius | M5III[68] | ||
U Herculis | 252.35[32] | Hercules | M6.5–M8[69] | ||
Sigma Canis Majoris | 258±21[14] – 272.15+12.22 −1.94[7] |
Canis Major | K5Ib[70] | ||
R Aquilae | 259±67 – 328±85[59] | Aquila | M6.5–M9e[71] | ||
R Cassiopeiae | 263[32] | Cassiopeia | M6.5e–M9.5e[72] | ||
Phi Cassiopeiae | 263[73] | Cassiopeia | F0Ia[74] | ||
Propus | 275+49 −66[3] |
Gemini | M3 III[3] | ||
T Ceti | 275[11] | Cetus | M5-6Se[75] | ||
Rasalgethi | 284±60 (264 – 303)[76] | Hercules | M5Ib-II[77] | May be the closest red supergiant to Earth[g] | |
XY Lyrae | 284.2[5][a] | Lyra | M4.5–M5II[78] | ||
V424 Lacertae | 288+26 −21[79] |
Lacerta | K5Ib[80] | ||
R Aquarii | 289.73[32]; 430[81] | Aquarius | M6.5–M8.5[82] | A symbiotic star. | |
TW Ophiuchi | 292[55] | Ophiuchus? | C-N5[83] | ||
Delta2 Lyrae | 292.5+19.3 −22.2[3] – 318[5][a] |
Lyra | M4 III[3] | Older papers give radii of 286 R☉[84] and 381 R☉.[85] | |
TX Piscium | 293[11] | Pisces | C7,2 | ||
R Hydrae | 297.2[32] | Hydra | M6e–M9e[86] | ||
X Ophiuchi | 298±78 – 314±81[59] | Ophiuchus | M0-8e[87] | ||
TW Horologii | 303[55] | Horologium | C | ||
RT Capricorni | 304[55] | Capricornus? | C | ||
S Coronae Borealis | 308.32[32] | Corona Borealis | M6.5e–M8.5e[88] | ||
Z Pegasi | 310±92[59] | Pegasus | M7-8e[89] | ||
5 Lacertae A | 319.2+26.6 −30[16] |
Lacerta | K9Ia[90] | ||
R Leonis | 320 – 350;[91] 324[32] | Leo | M7-M9e[92] | ||
Z Scorpii | 320±100[66] | Scorpius | M5.5e[93] | ||
Mira A | 332 – 402[94] | Cetus | M5–M9IIIe[95] | Prototype of the Mira variables. | |
W Hydrae | 339[23]–361.41[32] | Hydra | M7.5–M9e[23] | ||
La Superba | 342[h] | Canes Venatici | C–N5 B[97] | ||
BG Serpentis | 354±99[59] | Serpens | M7 D[98] | ||
R Sculptoris | 355±55[99] – 513[11] | Sculptor | C-N5+ B[100] | ||
SY Sculptoris | 358.1[32] | Sculptor | M6e[32] | ||
U Orionis | 370±96[59] | Orion | M6.5–M9.5e[101] | ||
R Cancri | 371±37[102] | Cancer | M6.5-M9e[103] | ||
PP Persei | 372+35 −23[79] |
Perseus | M0-M1.5I[104] | ||
T Indi | 372[55] | Indus | C | ||
S Vulpeculae | 382[105] | Vulpecula | K0[106] | ||
V509 Cassiopeiae | 390 – 910[107] | Cassiopeia | G0Ia0 (K5Ia0–A6Ia0)[107] | A yellow hypergiant. | |
RZ Sagittarii | 409[23] | Sagittarius | S4,4ep[108] | S-type star | |
S Orionis | 411–498[109] | Orion | M6.5–M7.5e[110] | ||
Y Cassiopeiae | 413±120[59] | Cassiopeia | M7.5e[111] | ||
T Cassiopeiae | 416±108[59] | Cassiopeia | M7–M9e[112] | ||
V810 Centauri A | 420[113] | Centaurus | F8Ia[113] | ||
U Antliae | 422.5[23] | Antlia | C-N3[23] | ||
LW Cygni | 445+13 −11[79] |
Cygnus | C5,4e[114] | ||
R Pegasi | 455±119 – 476±122[59] | Pegasus | M6–M8.5e[115] | ||
S Pegasi | 459±135 – 574±154[59] | Pegasus | M6-M8.5e[116] | ||
R Puppis | 477+28 −22[117] |
Puppis | G2-0 Ia[118] | A yellow hypergiant. | |
V382 Carinae | 485[119] | Carina | G5_0-Ia[120] | Brightest hypergiant in the sky. | |
V366 Andromedae | 492+39 −29[79] |
Andromeda | M2Ib[121] | ||
FZ Persei | 496+32 −28[79] |
Perseus | M1Iab[122] | ||
R Draconis | 511±142[59] | Draco | M4.5–M6+e[123] | ||
KK Persei | 513+22 −18[79] |
Perseus | M2Iab-Ib[124] | ||
RR Aquilae | 522+230 −140[102] |
Aquila | M7.5e[125] | ||
WY Geminorum A | 522+45 −34[79] |
Gemini | M2Iaebp[126] | ||
W Persei | 558+49 −30[79] |
Perseus | M3Iab-M5I[127] | ||
CW Leonis | 560[128] | Leo | C9,5e[129] | The nearest carbon star. | |
S Serpentis | 583±182 – 601±159[59] | Serpens | M5e[130] | ||
AD Persei | 594+49 −37[79] |
Perseus | M3Iab[131] | ||
W Orionis | 597[55] | Orion | C | ||
RR Persei | 599±161[59] | Perseus | M3+–M5e[132] | ||
UX Cygni | 608.14[32] | Cygnus | M6e–M6.5e[133] | ||
U Arietis | 610±125[66] | Aries | M4.5–M7.5e[134] | ||
SS Virginis | 425[55] | Virgo? | C | ||
Rho Cassiopeiae | 636 – 981[135] | Cassiopeia | G2Iae (F8pIa-K0pIa-0)[i] | A yellow hypergiant. | |
GX Monocerotis | 675+300 −249[102] |
Monoceros | M9[136] | ||
Antares | 680[137] | Scorpius | M1.5Iab[138] | 15th brightest star in the night sky. | |
BU Persei | 686+75 −57[79] |
Perseus | M4Ib[139] | ||
R Volantis | 687[55] | Volans | C |
Notes
- ^ a b c d e f g h i Radius from temperature and bolometric magnitude. The bolometric magnitude is converted to solar luminosites in the equation (L = 10^(0.4*(4.74-(Mbol)))), where L is the luminosity and Mbol the bolometric magnitude
- ^ Radius calculated with a temperature of 4146 K and a luminosity of 4079.74 L☉.
- ^ Radius calculated from an angular diameter of 7.004 mas and a distance of 200.369 parsecs.
- ^ From angular diameters of 5.65±0.5 and 4.13±0.27 milliarcseconds and a distance of 277 parsecs, which is calculated from the parallax of 3.61 milliarcseconds.
- ^ see the Gamma Cygni article
- ^ Radii calculatei using angular diameters of 3.29±0.66 and 3.457±0.024 mas respectively, together with a Hipparcos distance of 550 parsecs.
- ^ See List of nearest supergiants
- ^ From an angular diameter of 13.81 mas [96] and a distance of 230 parsecs.
- ^ See the Rho Cassiopeiae article
References
- ^ Observations and Interpretation of Luminous Blue Variables
- ^ "S Dor". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h i j k l m n Angular Diameters and Fundamental Parameters of Forty-Four Stars from the Navy Precision Optical Interferometer
- ^ a b c Hubble Space Telescope Constraints on the Winds and Astrospheres of Red Giant Stars
- ^ a b c d e f g h i j Exploring masses and CNO surface abundances of red giant stars
- ^ "Scheat". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f Precise radial velocities of giant stars. X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search. Avaliable here in VizieR.
- ^ "Sigma Ophiuchi". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Mu Geminorum". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b Physical Parameters and Wind Properties of Galactic Early B Supergiants
- ^ a b c d e f Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ "V378 Normae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
- ^ "Epsilon Muscae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer
- ^ Fundamental parameters and infrared excesses of Hipparcos stars.
- ^ A catalogue of stellar diameters and fluxes for mid-infrared interferometry. Data can be accessed here at VizieR.
- ^ "Iota Aurigae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "V337 Carinae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ CHARM2: An updated Catalog of High Angular Resolution Measurements. Data can be seen here at VizieR. Select the first table, query the selected table. Later, select all columns and submit, type a SAO or IRC designation in "Id1" and submit.
- ^ a b Spitzer Spectroscopy of Dusty Disks around B e Hypergiants in the Large Magellanic Cloud
- ^ a b c d e f g h i j k l far-UV emission surrounding asymptotic giant branch stars as seen by GALEX
- ^ "Tiaki". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "GZ Velorum". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Rho Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Interferometry of ɛ Aurigae: Characterization of the Asymmetric Eclipsing Disk
- ^ Recent UBVJH Photometry of Epsilon Aurigae
- ^ "Epsilon Aurigae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ α TrA Junior
- ^ "Atria". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h i j k l m n o A Method to Estimate the Masses of Asymptotic Giant Branch Variable Stars
- ^ "HD 56096". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "HD 210762". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Omega Capricorni". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Observations of the pulsation of the Cepheid l Car with the Sydney University Stellar Interferometer
- ^ "HD 84810". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Zeta Cephei". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ 33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble
- ^ "Gamma Cygni". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "30 Her". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Lyrae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "72 Leo". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "24 Sgr". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "OP Herculis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Quantitative spectroscopy of Deneb
- ^ "Deneb". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b Cite error: The named reference
:5
was invoked but never defined (see the help page). - ^ "Epsilon Pegasi". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "NS Pup". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "S Crateris". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "omi01 ori". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ The Emergent Flux and Effective Temperature of Delta Canis Majoris
- ^ "Delta Canis Majoris". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h i Dust emission modelling of AGB stars
- ^ "NP Pup". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "62 Cyg". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "W Cygni". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h i j k l m Angular Size Measurements Of Mira Variable Stars At 2.2 Microns. II
- ^ "BG Cyg". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "RX Boo". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Infrared Interferometric Three-dimensional Diagnosis of the Atmospheric Dynamics of the AGB Star R Dor with VLTI/AMBER
- ^ JD13 – Eta Carinae in the Context of the Most Massive Stars
- ^ "Eta Carinae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Carinae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c Angular diameter measurements of evolved variables by lunar occultations at 2.2 and 3.8 micron
- ^ "SW Virginis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "70 Sgr". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "U Her". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "sig CMa". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Aql". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Cas". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ A determination of the basic atmospheric parameters of Phi Cassiopeiae
- ^ "Phi Cassiopeiae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "T Ceti". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ The Age and Mass of the α Herculis Triple-star System from a MESA Grid of Rotating Stars with 1.3 <= M/M ⊙ <= 8.0
- ^ "Alpha Herculis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "XY Lyrae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c d e f g h i j Ryan Norris. "Student Science at NMT: Learning Optical Interferometry Through Projects on Evolved Stars" (PDF). CHARA.
- ^ "V424 Lac". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ The spectroscopic orbit and the geometry of R Aquarii".
- ^ "R Aqr". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "TW Oph". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Isotopic abundances of Carbon and Oxygen in Oxygen-rich giant stars
- ^ Really Cool Stars and the Star Formation History at the Galactic Center
- ^ "R Hydrae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "X Oph". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "S CrB". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Z Peg". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "5 Lacertae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ The K -Band Intensity Profile of R Leonis Probed by VLTI/VINCI
- ^ "R Leonis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Z Sco". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared
- ^ "Mira". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Angular diameters of the carbon stars UU Aurigae, Y Canum Venaticorum, and TX PISCIUM from optical long-baseline interferometry
- ^ "La Superba". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "BG Ser". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Aperture synthesis imaging of the carbon AGB star R Sculptoris. Detection of a complex structure and a dominating spot on the stellar disk
- ^ "R Scl". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "U Ori". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c New insights into the dust formation of oxygen-rich AGB stars
- ^ "R Cnc". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "PP Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Cepheid Period‐Radius and Period‐Luminosity Relations and the Distance to the Large Magellanic Cloud
- ^ "S Vulpeculae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b The hypergiant HR 8752 evolving through the yellow evolutionary void
- ^ "RZ Sgr". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ The Mira variable S Orionis: Relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs
- ^ "S Orionis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "Y Cas". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "T Cassiopeiae". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b The pulsating yellow supergiant V810 Centauri
- ^ "LW Cyg". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Peg". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "S Peg". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ "R Pup". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Analysing the spectral energy distributions of Galactic classical Cepheids
- ^ "V382 Car". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "V366 And". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "FZ Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Dra". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "KK Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "RR Aql". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "WY Gem". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "W Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Herschel/HIFI observations of the circumstellar ammonia lines in IRC+10216
- ^ "CW Leo". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "S Serpentis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "AD Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "R Per". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "UX Cygni". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "U Arietis". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Pulsations, eruptions, and evolution of four yellow hypergiants
- ^ "GX Mon". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER
- ^ "Antares". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ "BU Per". SIMBAD. Centre de données astronomiques de Strasbourg.