NGC 752

{{Short description|Open cluster in the constellation Andromeda}}

{{Infobox cluster

| image =File:NGC_752.png

| caption = NGC 752

| credit =

| name = NGC 752

| constellation = Andromeda

| type =

| epoch = J2000

| ra = {{RA|01|57|41}}{{cite simbad|title=NGC 752|access-date=10 February 2018}}

| dec = {{DEC|+37|47.1}}

| dist_ly = 1,470 ly{{cite conference |bibcode=2022csss.confE..82G |title=Open cluster NGC752: Revision by GAIA EDR3 data |last1=Gaysin |first1=Renat |last2=Hojaev |first2=Alisher |journal=Cambridge Workshop on Cool Stars |year=2022 |page=82 |doi=10.5281/zenodo.7481659 }}

| dist_pc = 450 pc

| appmag_v = 5.7{{cite book | last = Dunlop | first = Storm | author-link = Storm Dunlop | title = Atlas of the Night Sky | url = https://archive.org/details/collinsatlasofni0000dunl | url-access = registration | publisher = Collins | year = 2005 | isbn = 978-0-00-717223-8}}

| size_v = 75{{prime}}

| radius_ly =

| absmag_v =

| constellation name = Andromeda

| notes =

| names = Caldwell 28, Cr 23

}}

File:NGC 752 map.png

NGC 752 (also known as Caldwell 28) is an open cluster in the constellation Andromeda. The cluster was discovered by Caroline Herschel in 1783 and cataloged by her brother William Herschel in 1786, although an object that may have been NGC 752 was described by Giovanni Batista Hodierna before 1654.{{cite web|url=http://cseligman.com/text/atlas/ngc7a.htm#752|title=New General Catalogue objects: NGC 750 - 759|author=Seligman, Courtney|website=cseligman.com|access-date=10 February 2018}}

The large cluster lies 1,400 light-years away from the Earth and is easily seen through binoculars, although it may approach naked eye visibility under good observing conditions. A telescope reveals about 60 stars no brighter than 9th magnitude within NGC 752.Frommert, Kronberg, [http://messier.seds.org/xtra/ngc/n0752.html SEDS: NGC 752]

Components

The most up-to-date research lists 302 stars as members of NGC 752. Since the age of the cluster is {{val|1.34|0.06|ul=Gyr}}, they are mainly low mass stars on the main sequence or red giants, with a main sequence turnoff at about F0. A blue straggler star is also present, along with some spectroscopic binaries and variable stars. The detached eclipsing binary DS Andromedae is a member of this cluster.{{cite journal|arxiv=2210.11649|doi=10.3847/1538-3881/ac9c59 |title=Evolved Eclipsing Binaries and the Age of the Open Cluster NGC 752 |year=2023 |last1=Sandquist |first1=Eric L. |last2=Buckner |first2=Andrew J. |last3=Shetrone |first3=Matthew D. |last4=Barden |first4=Samuel C. |last5=Pilachowski |first5=Catherine A. |last6=Deliyannis |first6=Constantine P. |last7=Harmer |first7=Dianne |last8=Mathieu |first8=Robert |last9=Meibom |first9=Søren |last10=Frandsen |first10=Søren |last11=Orosz |first11=Jerome A. |journal=The Astronomical Journal |volume=165 |issue=1 |page=6 |bibcode=2023AJ....165....6S |s2cid=253080539 |doi-access=free }}

Images

=Notable stars=

border="0" cellpadding="6" cellspacing="1" style="margin-right:0.4em; background:#CDC9C9;"

! colspan="1" | Name

Right ascensionDeclinationApparent magnitude (V)Spectral typeDatabase referencesRelevance
bgcolor="#FFFAFA"

| TYC 2816-327-1

01h 56m 08.9572s+37° 39' 52.7528"10.41F5.3V[http://simbad.u-strasbg.fr/simbad/sim-id?protocol=html&Ident=TYC+2816-327-1 Simbad]Gamma Doradus variable
bgcolor="#FFFAFA"

| DS Andromedae

01h 57m 46.0561s+38° 04' 28.43112"10.44 - 10.93 (variable)F3IV-V + G0V (double)[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=DS+And Simbad]Beta Lyrae variable
bgcolor="#FFFAFA"

| BD+37 416

01h 56m 10.3002s+37° 45' 00.0301"10.00F2III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+416 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+37 416B

01h 56m 11.1020s+37° 45' 11.3889"11.19F0[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+416B Simbad]Candidate companion of BD+37 416
bgcolor="#FFFAFA"

| TYC 2816-1390-1

01h 56m 12.8772s+38° 01' 43.1869"10.88F3V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=TYC+2816-1390-1 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| TYC 2319-568-1

01h 56m 57.5899s+37° 23' 20.6538"10.6F2V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=TYC+2319-568-1 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| 2MASS J01571216+3756048

01h 57m 12.1584s+37° 56' 04.7909"11.9G5.0V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J01571216%2B3756048 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+36 364

01h 57m 25.9968s+37° 43' 19.6966"10.4F2III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B36+364 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| QX Andromedae

01h 57m 57.7818s+37° 48' 22.4500"11.28 - 11.50 (variable)F5[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=QX+Andromedae Simbad]W Ursae Majoris variable
bgcolor="#FFFAFA"

| 2MASS J01575883+3741269

01h 57m 58.8386s+37° 41' 26.9575"12.31F8[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J01575883%2B3741269 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| TYC 2816-691-1

01h 58m 16.8604s+37° 38' 15.9955"11.21F5V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=TYC+2816-691-1 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| V447 Andromedae

01h 58m 53.9322s+37° 34' 42.5263"13.39K3.0[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=V447+And Simbad]RS Canum Venaticorum variable
bgcolor="#FFFAFA"

| BD+36 348

01h 55m 27.6831s+37° 34' 04.6482"10.14F2V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B36+348 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+37 410

01h 55m 29.2926s+37° 50' 26.3171"9.94F4III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+410 Simbad]Eclipsing binary
bgcolor="#FFFAFA"

| BD+37 418

01h 56m 18.8954s+37° 58' 00.4602"8.97G9III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+418 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| HD 11812

01h 56m 49.7623s+38° 01' 21.6883"9.13F3V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+11812 Simbad]In the HD catalogue
bgcolor="#FFFAFA"

| HD 11811

01h 56m 50.4330s+38° 01' 58.1400"8.91G2V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+11811 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+37 431

01h 57m 36.2116s+37° 45' 10.1549"9.85F2III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+431 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+36 367

01h 57m 37.3494s+37° 29' 27.6181"9.75A0III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B36+367 Simbad]Blue straggler
bgcolor="#FFFAFA"

| BD+36 368

01h 57m 37.5965s+37° 39' 37.9032"8.85K1III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B36+368 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+37 439

01h 57m 59.3462s+37° 54' 53.9679"9.85F2III[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+439 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| BD+37 444

01h 58m 36.8870s+37° 45' 10.7241"9.62F2V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD%2B37+444 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| TYC 2816-771-1

01h 58m 40.0620s+37° 38' 05.2030"12.43F2V[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=TYC+2816-771-1 Simbad]Spectroscopic binary
bgcolor="#FFFAFA"

| 2MASS J01591990+3723230

01h 59m 19.8967s+37° 23' 23.0364"12.893[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J01591990%2B3723230 Simbad]Spectroscopic binary

References

{{Reflist| refs=

{{cite journal |title=A New Look at an Old Cluster: The Membership, Rotation, and Magnetic Activity of Low-mass Stars in the 1.3 Gyr Old Open Cluster NGC 752 |journal=The Astrophysical Journal | last1=Agüeros |first1=M. A. | last2= Bowsher |first2=E. C. |last3=Bochanski |first3=J. J. |last4=Cargile |first4=P. A. |last5=Covey |first5=K. R. |last6=Douglas |first6=S. T. |last7=Kraus |first7=A. |last8=Kundert |first8=A. |last9=Law |first9=N. M. |last10=Ahmadi |first10=A. |last11=Arce |first11=H. G. |volume=862 |issue=1 |pages=33 |date=July 2018 |bibcode=2018ApJ...862...33A|doi=10.3847/1538-4357/aac6ed |arxiv=1804.02016 |s2cid=119438236 |doi-access=free }}

{{cite journal |title=Soft X-rays from the intermediate-age open cluster NGC 752 |journal=Astronomy and Astrophysics | last1=Belloni |first1=T. | last2=Verbunt |first2=F. |volume=305 |pages=806 |date=January 1996 |bibcode=1996A&A...305..806B}}

}}