Променлива ѕвезда од типот на Алфа Лебед: Разлика помеѓу преработките

| 2^м,38

| 2^м,48

| B5Ia

| 105.000<ref name=an331_4_349>{{citation | last1=Hohle | first1=M. M. | last2=Neuhäuser | first2=R. | last3=Schutz | first3=B. F. | title=Masses and luminosities of O- and B-type stars and red supergiants | journal=Astronomische Nachrichten | volume=331 | issue=4 | page=349 |date=April 2010 | doi=10.1002/asna.200911355 | bibcode=2010AN....331..349H |arxiv = 1003.2335 }}</ref>

| 2^м,98

| 3^м,04

| B3Ia

| 219.000<ref name=crowther/>

| 4^м,12

| 4^м,21

| B1Ia

| 331.000<ref name=crowther/>

| 5^м,12

| 5^м,22

| A2Ia

| 136.000<ref name="Kaufer 1996">{{наведено списание|author=Kaufer, A.|author2=Stahl, O.|author3=Wolf, B.|author4=Gaeng, T.|author5=Gummersbach, C. A.|author6=Kovacs, J.|author7=Mandel, H.|author8=Szeifert, T.|date=1996|title=Long-term spectroscopic monitoring of BA-type supergiants. I. Halpha_ line-profile variability.|journal=Astronomy and Astrophysics|volume=305|pages=887–901 | bibcode=1996A&A...305..887K}}</ref>

| 6^м,24

| 6^м,28

| B1.5Ia

| 242.000<ref name=lamers1995>{{наведено списание|last1=Lamers|first1=Henny J. G. L. M.|last2=Snow|first2=Theodore P.|last3=Lindholm|first3=Douglas M.|title=Terminal Velocities and the Bistability of Stellar Winds|journal=The Astrophysical Journal|volume=455|date=1995|pages=269|issn=0004-637X|doi=10.1086/176575|bibcode = 1995ApJ...455..269L }}</ref>

| 4^м,19

| 4^м,26

| B9 Iab

| 39.000<ref name="MarkovaPuls2008">{{наведено списание|last1=Markova|first1=N.|last2=Puls|first2=J.|title=Bright OB stars in the Galaxy|journal=Astronomy and Astrophysics|volume=478|issue=3|date=2008|pages=823–842|issn=0004-6361|doi=10.1051/0004-6361:20077919|arxiv = 0711.1110 |bibcode = 2008A&A...478..823M }}</ref>

| 5^м,75

|

| B3 Ia

| 200.000<ref>{{наведено списание|bibcode=1999A&A...350..970K|arxiv = astro-ph/9910449 |title = The wind momentum-luminosity relationship of galactic A- and B-supergiants |journal = Astronomy and Astrophysics |volume = 350 |pages = 970 |last1 = Kudritzki |first1 = R. P. |last2 = Puls |first2 = J. |last3 = Lennon |first3 = D. J. |last4 = Venn |first4 = K. A. |last5 = Reetz |first5 = J. |last6 = Najarro |first6 = F. |last7 = McCarthy |first7 = J. K. |last8 = Herrero |first8 = A. |date = 1999 }}</ref>

| 3^м,83

| 3^м,9

| B1Iab

| 295.000<ref name=crowther/>

| 0^м,17

| 0^м,22

| B8Ia

| 279.000<ref name="Chesneau 2014"/><br>

| 1^м,64

| 1^м,74

| B0.5Iabea

| 275.000<ref name=crowther/><br>

| 4^м,68

| 4^м,72

| B2Ia

| 446.000<ref name=crowther>{{наведено списание | last1 = Crowther | first1 = P. A. | last2 = Lennon | first2 = D. J. | last3 = Walborn | first3 = N. R. | title = Physical parameters and wind properties of galactic early B supergiants | doi = 10.1051/0004-6361:20053685 | journal = Astronomy and Astrophysics | volume = 446 | issue = 1 | pages = 279–293 | date = 2006 |arxiv = astro-ph/0509436 |bibcode = 2006A&A...446..279C }}</ref>