DM Ursae Majoris
{{Short description|Variable star in the constellation Ursa Major}}
{{Starbox begin}}
{{Starbox image
| image = 250px
| caption = Visual band light curves for DM Ursae Majoris, adapted from Mohin et al. (1985)
}}
{{Starbox observe
| epoch = J2000
| constell = Ursa Major
}}
{{Starbox character
| type =
| class = K0III-IV {{nowrap|(K0IV + K5V)}}
| variable = RS CVn
}}
{{Starbox astrometry
| prop_mo_ra = −37.912
| prop_mo_dec = −7.566
| parallax = 5.3862
| p_error = 0.0157
}}
{{Starbox orbit
| primary =
| name =
| period =
| period_unitless = {{val|7.4920|0.0009|u=days|fmt=commas}}
| axis =
| axis_unitless =
| eccentricity = 0.0 (assumed)
| node =
| periastron = {{val|2443881.4|0.1|ul=JD|fmt=commas}}
| periarg = 0.0 (assumed)
| periarg_primary =
| k1 = 27.6
| k2 =
}}
{{Starbox detail
| source =
| component1 = Primary
| gravity =
| metal_fe =
| rotational_velocity =
| age_myr =
| component2 = Secondary
}}
{{Starbox catalog
| names = {{odlist | name=2A 1052+606 | V=DM UMa | BD=+61°1211 | HIP=53425 | PPM=17646 | SAO=15338 }}
}}
{{Starbox reference
| Simbad = DM+UMa
}}
{{Starbox end}}
DM Ursae Majoris is a binary star system in the northern circumpolar constellation of Ursa Major, abbreviated DM UMa. It is sometimes identified by the Bonner Durchmusterung catalogue designation {{nowrap|BD +61 1211}}; DM UMa is the variable star designation. The system has a combined apparent visual magnitude of 9.29, which is too faint to be visible to the naked eye. Based on parallax measurements, the system is located at a distance of approximately 606 light years from the Sun, but it is drifting closer with a heliocentric radial velocity of −7 km/s.
In 1978, the X-ray source designated 2A 1052+606 was initially included in the 2A catalogue of observations by the Ariel 5 satellite. The approximate position of this source was determined using the HEAO-1 satellite, then W. Liller matched it with the candidate star SAO 015338 (later DM UMa). He determined the spectra matches a K-type star with strong H-alpha emission lines. In 1979, this object was shown to be an RS Canum Venaticorum variable (RS CVn) by D. Crampton and associates, which indicated this is a close binary star system where one of the components has an active chromosphere with star spots. DM UMa was the first RS CVn variable to be so classified based on its X-ray emission.
Radial velocity measurements demonstrated an orbital period of about 7.5 days. A mass function of {{val|0.016|ul=Solar mass}} suggested the system is being viewed from a low inclination, close to pole-on. The system showed variations in emission lines on a time scale of a day. A photometric light curve was generated by R. A. Kimble and associates in 1981, showing strong variability within each orbital period. A model fit to the light curve indicated the star has an extensive distribution of star spots, with regions of enhanced spot activity toward and away from the companion. It is one of the few variables of this class that show a continual emission of H-alpha, although this varies by a factor of three over the course of an orbit.
This is a single-lined spectroscopic binary with the spectra matching a stellar classification of K0III-IV. The secondary is at least 1.5 magnitudes fainter than the primary, so the contribution of the former to the luminosity is no more than 20%. The observed properties of the system can be modeled by a combination of a subgiant primary of class K0IV with a K5V main sequence secondary.
References
{{reflist|refs=
{{cite simbad | title=DM UMa | access-date=2022-10-01 }}
{{Cite Gaia EDR3|861644351670829568}}
| display-authors=1 | last1=Samus | first1=N. N.
| last2=Kazarovets | first2=E. V. | last3=Durlevich | first3=O. V.
| last4=Kireeva | first4=N. N. | last5=Pastukhova | first5=E. N.
| title=General Catalogue of Variable Stars
| version=5.1 | journal=Astronomy Reports
| year=2017 | volume=61 | issue=1 | pages=80–88
| bibcode=2017ARep...61...80S | doi=10.1134/S1063772917010085
| s2cid=125853869 | postscript=. }}
| title=Starspots | postscript=.
| last=Strassmeier | first=Klaus G.
| journal=The Astronomy and Astrophysics Review
| volume=17 | issue=3 | pages=251–308 | date=September 2009
| doi=10.1007/s00159-009-0020-6 | bibcode=2009A&ARv..17..251S | doi-access=free }}
| last1=Mohin | first1=S. | last2=Raveendran | first2=A. V.
| last3=Mekkaden | first3=M. V. | last4=Hall | first4=D. S.
| last5=Henry | first5=G. W. | last6=Lines | first6=R. D.
| last7=Fried | first7=R. E. | last8=Louth | first8=H.
| last9=Stelzer | first9=H. J.
| title=Evolution of Starspot Regions in DM UMa
| journal=Astrophysics and Space Science | date=October 1985 | volume=115 | issue=2
| pages=353–368 | doi=10.1007/BF00653812 | bibcode=1985Ap&SS.115..353M
| s2cid=119914476 | url=https://articles.adsabs.harvard.edu/pdf/1985Ap%26SS.115..353M | access-date=6 October 2022}}
| title=The RS CVn system BD +61 1211 = 2A 1052+60.6
| display-authors=1 | last1=Crampton | first1=D.
| last2=Dobias | first2=J. | last3=Margon | first3=B.
| journal=Astrophysical Journal
| volume=234 | pages=993–996 | date=December 1979
| doi=10.1086/157583 | bibcode=1979ApJ...234..993C | s2cid=120565755 | url=https://nrc-publications.canada.ca/eng/view/accepted/?id=8d28418a-1a11-4d39-bbe7-0cf1671603e9 }}
| title=2A 1052+606 = SAO 015338?
| last1=Liller | first1=W. | last2=McCrosky | first2=R. E.
| last3=Gursky | first3=H. | last4=Griffiths | first4=R.
| display-authors=1 | journal=IAU Circular
| volume=3176 | page=2 | date=February 1978
| editor-last=Marsden | editor-first=B. G.
| bibcode=1978IAUC.3176....2L }}
| title=The Ariel V (SSI) catalogue of high galactic latitude ({{pipe}}b{{pipe}} > 10°) X-ray sources
| display-authors=1 | last1=Cooke | first1=B. A.
| last2=Ricketts | first2=M. J. | last3=Maccacaro | first3=T.
| last4=Pye | first4=J. P. | last5=Elvis | first5=M.
| last6=Watson | first6=M. G. | last7=Griffiths | first7=R. E.
| last8=Pounds | first8=K. A. | last9=McHardy | first9=I.
| last10=Maccagni | first10=D. | last11=Seward | first11=F. D.
| last12=Page | first12=C. G. | last13=Turner | first13=M. J. L.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=182 | pages=489–515 | date=February 1978
| issue=3
| doi=10.1093/mnras/182.3.489 | bibcode=1978MNRAS.182..489C | doi-access=free }}
| title=X-ray and optical variability in 2A1052+606-a new RS CVn-type system
| display-authors=1 | last1=Charles | first1=P.
| last2=Walter | first2=F. | last3=Bowyer | first3=S.
| journal=Nature | volume=282 | issue=5740 | pages=691–692 | date=December 1979
| doi=10.1038/282691a0 | bibcode=1979Natur.282..691C | s2cid=4315279
}}
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| title=XHIP: An extended hipparcos compilation
| journal=Astronomy Letters
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | arxiv=1108.4971
| doi=10.1134/S1063773712050015 | s2cid=119257644 }}
{{citation | postscript=. | display-authors=1
| title=Spot activity in the RS CVn binary DM Ursae Majoris
| last1=Rosario | first1=M. J. | last2=Heckert | first2=P. A.
| last3=Mekkaden | first3=M. V. | last4=Raveendran | first4=A. V.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=394 | issue=2 | pages=872–881 | date=April 2009
| doi=10.1111/j.1365-2966.2008.14372.x | doi-access=free
| bibcode=2009MNRAS.394..872R | s2cid=123218100
}}
| title=Discovery of a large-amplitude photometric wave in the RS CVn binary BD +61 1211 (=DM UMA) and constraints on starspot models for the observed variation
| display-authors=1 | last1=Kimble | first1=R. A.
| last2=Kahn | first2=S. M. | last3=Bowyer | first3=S.
| journal=Astrophysical Journal
| volume=251 | pages=585–590 | date=December 1981
| doi=10.1086/159502 | bibcode=1981ApJ...251..585K }}
| title=Spot and Chromospheric Activity on the RS CVN Star DM Ursae Majoris
| last=Hatzes | first=Artie P.
| journal=Astronomical Journal
| volume=109 | page=350 | date=January 1995
| doi=10.1086/117280 | bibcode=1995AJ....109..350H | doi-access=free}}
}}
Further reading
{{Div col|small=yes}}
- {{citation | postscript=.
| title=Chromospheric activity on late-type star DM UMa using high-resolution spectroscopic observations
| display-authors=1 | last1=Zhang | first1=LiYun
| last2=Pi | first2=QingFeng | last3=Han | first3=Xianming L.
| last4=Chang | first4=Liang | last5=Wang | first5=Daimei
| journal=Monthly Notices of the Royal Astronomical Society
| volume=459 | issue=1 | pages=854–862
| date=June 2016 | doi=10.1093/mnras/stw668
| doi-access=free
| arxiv=1611.07395 | bibcode=2016MNRAS.459..854Z }}
- {{citation | postscript=.
| title=A New Approach to the Long-Term Activity Behavior of DM UMa
| last1=Taş | first1=G. | last2=Evren | first2=S.
| journal=Baltic Astronomy
| volume=21 | pages=435–446 | year=2012
| issue=4
| doi=10.1515/astro-2017-0401 | bibcode=2012BaltA..21..435T | s2cid=46781397
| doi-access=free}}
- {{citation | postscript=.
| title=Near simultaneous BV photometry and Hα spectroscopy of the RS Canum Venaticorum binary DM Ursae Majoris
| last1=Mohin | first1=S. | last2=Raveendran | first2=A. V.
| journal=Astronomy and Astrophysics
| volume=286 | pages=824–828 | date=June 1994
| bibcode=1994A&A...286..824M }}
- {{citation | postscript=.
| title=Photometric study of the RS CVn binary DM Ursa Majoris
| last1=Mohin | first1=S. | last2=Raveendran | first2=A. V.
| journal=Astronomy and Astrophysics
| volume=256 | pages=487–494 | date=March 1992
| bibcode=1992A&A...256..487M }}
- {{citation | postscript=.
| title=1988 and 1989 UBV Photometry of BD +61 1211
| last=Heckert | first=P. A.
| journal=Information Bulletin on Variable Stars
| volume=3446 | page=1 | date=March 1990
| bibcode=1990IBVS.3446....1H }}
- {{citation | postscript=.
| title=UBV Photometry of BD +61 1211 during 1986 and 1987
| display-authors=1 | last1=Heckert | first1=P. A.
| last2=Summers | first2=D. | last3=Harkey | first3=R.
| last4=Sandoval | first4=V. | last5=Pilkey | first5=C.
| journal=Information Bulletin on Variable Stars
| volume=3274 | page=1 | date=December 1988
| bibcode=1988IBVS.3274....1H }}
- {{citation | postscript=.
| title=UBV Photometry of BD + 611211 and HD 80715 During 1986 and 1987
| display-authors=1 | last1=Heckert | first1=P. A.
| last2=Summers | first2=D. | last3=Harkey | first3=R.
| last4=Sandoval | first4=V. | last5=Pilkey | first5=C.
| journal=Bulletin of the American Astronomical Society
| volume=20 | page=674 | date=March 1988
| bibcode=1988BAAS...20..674H }}
- {{citation | postscript=.
| title=Hα observations of RS Canum Venaticorum stars. II. 1981 observations for UX Arietis, HR 1099, and BD +61°1211
| last1=Nations | first1=Harold L. | last2=Ramsey | first2=Lawrence W.
| journal=Astronomical Journal
| volume=92 | pages=1403–1408 | date=December 1986
| doi=10.1086/114274 | bibcode=1986AJ.....92.1403N }}
- {{citation | postscript=.
| title=Hα Observations of RS CVn Stars: 1981 Spectra of UX Ari, HR 1099, BD +61 1211 and HD 155638
| last1=Nations | first1=H. L. | last2=Ramsey | first2=L. W.
| journal=Bulletin of the American Astronomical Society
| volume=17 | page=754 | date=June 1985
| bibcode=1985BAAS...17..754N }}
- {{citation | postscript=.
| title=Halpha Emission in RS CVn Stars: BD +61 1211 and HD 37847
| last1=Tan | first1=Huisong | last2=Liu | first2=Xuefu
| journal=Information Bulletin on Variable Stars
| volume=2669 | page=1 | date=February 1985
| doi=10.1086/157583
| bibcode=1979ApJ...234..993C | s2cid=120565755
| url=https://nrc-publications.canada.ca/eng/view/accepted/?id=8d28418a-1a11-4d39-bbe7-0cf1671603e9
}}
{{Div col end}}
{{Stars of Ursa Major}}
Category:K-type main-sequence stars
Category:RS Canum Venaticorum variables