THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33

ABSTRACT   549 blue stars with Ho; excess in the galaxy M 33 selected as candidates into unique objects of SS 433 and LBV (luminous blue variables) types are studied. These objects were divided by morphological types on Hog images in the following way: 81 stars, 154 diffuse nebulae, 180 bubble-type...

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Main Author: O. N. Sholukhova
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-08-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/109046
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author O. N. Sholukhova
author_facet O. N. Sholukhova
author_sort O. N. Sholukhova
collection DOAJ
description ABSTRACT   549 blue stars with Ho; excess in the galaxy M 33 selected as candidates into unique objects of SS 433 and LBV (luminous blue variables) types are studied. These objects were divided by morphological types on Hog images in the following way: 81 stars, 154 diffuse nebulae, 180 bubble-type nebulae and 117 common intermediate objects. The diffuse objects are Hll regions with an exciting star. The bubbles are probably the envelopes around WR stars or the remnants of supernovae. Among the stars a group of 20 brightest ones is selected which by their average properties agree satisfactory with the parameters of blue super-supergiants or the objects of LBV type. The interstellar absorption determined by bright stars is equal to AV = 0.93 ± 0.05.
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spelling doaj.art-129f75676e994a989d9e46bfcb17bff02022-12-22T03:00:35ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-08-0190535410.18524/1810-4215.1996.9.109046109046THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33O. N. Sholukhova0Special Astrophysical ObservatoryABSTRACT   549 blue stars with Ho; excess in the galaxy M 33 selected as candidates into unique objects of SS 433 and LBV (luminous blue variables) types are studied. These objects were divided by morphological types on Hog images in the following way: 81 stars, 154 diffuse nebulae, 180 bubble-type nebulae and 117 common intermediate objects. The diffuse objects are Hll regions with an exciting star. The bubbles are probably the envelopes around WR stars or the remnants of supernovae. Among the stars a group of 20 brightest ones is selected which by their average properties agree satisfactory with the parameters of blue super-supergiants or the objects of LBV type. The interstellar absorption determined by bright stars is equal to AV = 0.93 ± 0.05.http://oap.onu.edu.ua/article/view/109046
spellingShingle O. N. Sholukhova
THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33
Odessa Astronomical Publications
title THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33
title_full THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33
title_fullStr THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33
title_full_unstemmed THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33
title_short THE SEARCH FOR SS433 OBJECTS: Hα PHOTOMETRY OF BLUE STARS IN M33
title_sort search for ss433 objects hα photometry of blue stars in m33
url http://oap.onu.edu.ua/article/view/109046
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