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Am star in the constellation Delphinus
HD 193472 (HR 7774) is a solitary
star in the equatorial
constellation
Delphinus. It has an
apparent magnitude of 5.94,
[2] making it visible with the
naked eye if viewed under ideal conditions.
Parallax measurements put it at a distance of 282
light years
[1] and has a
radial velocity of −8
km/s,
[5] indicating that the object drifting towards the
Solar System.
HD 193472 has a
stellar classification of kA4 hF0 mF2,
[3] indicating that its an
Am star with the
calcium K-line of an A4 star, the
hydrogen lines and
effective temperature of a F0 star, and the metallic lines of a F2 star. Due to a radius over three times that of the
Sun and a relatively low
surface gravity, it appears to be slightly evolved. HD 193472 has 161% the
mass of the Sun and shines at 24 times the
luminosity of the Sun
[11] from its
photosphere at an
effective temperature of 7,188
K, giving it a yellowish white glow. HD 193472 has a
projected rotational velocity of 105
km/s.
[9]
References
- ^
a
b
c
d
e
Brown, A. G. A.; et al. (Gaia collaboration) (2021).
"Gaia Early Data Release 3: Summary of the contents and survey properties".
Astronomy & Astrophysics. 649: A1.
arXiv:
2012.01533.
Bibcode:
2021A&A...649A...1G.
doi:
10.1051/0004-6361/202039657.
S2CID
227254300. (Erratum:
doi:
10.1051/0004-6361/202039657e).
Gaia EDR3 record for this source at
VizieR.
- ^
a
b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30.
Bibcode:
2000A&A...355L..27H.
ISSN
0004-6361.
- ^
a
b Abt, Helmut A.; Morrell, Nidia I. (July 1995).
"The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135.
Bibcode:
1995ApJS...99..135A.
doi:
10.1086/192182.
ISSN
0067-0049.
- ^
a
b Mendoza, E. E.; Gomez, V. T.; Gonzalez, S. (June 1978).
"UBVRI photometry of 225 AM stars". The Astronomical Journal. 83: 606.
Bibcode:
1978AJ.....83..606M.
doi:
10.1086/112242.
ISSN
0004-6256.
- ^
a
b Kharchenko, N.V.; Scholz, R.-D.; Piskunov, A.E.; Röser, S.; Schilbach, E. (November 2007).
"Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations". Astronomische Nachrichten. 328 (9): 889–896.
arXiv:
0705.0878.
Bibcode:
2007AN....328..889K.
doi:
10.1002/asna.200710776.
ISSN
0004-6337.
-
^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346.
arXiv:
1108.4971.
Bibcode:
2012AstL...38..331A.
doi:
10.1134/S1063773712050015.
ISSN
1063-7737.
S2CID
255204555.
- ^
a
b
c
d
e Stassun, Keivan G.; et al. (2019-10-01).
"The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138.
arXiv:
1905.10694.
Bibcode:
2019AJ....158..138S.
doi:
10.3847/1538-3881/ab3467.
hdl:
1721.1/124721.
ISSN
0004-6256.
S2CID
166227927.
-
^ Gáspár, András; et al. (2016).
"The Correlation between Metallicity and Debris Disk Mass". The Astrophysical Journal. 826 (2): 171.
arXiv:
1604.07403.
Bibcode:
2016ApJ...826..171G.
doi:
10.3847/0004-637X/826/2/171.
S2CID
119241004.
- ^
a
b Royer, F.; Grenier, S.; Baylac, M.-O.; Gómez, A. E.; Zorec, J. (October 2002).
"Rotational velocities of A-type stars". Astronomy & Astrophysics. 393 (3): 897–911.
arXiv:
astro-ph/0205255.
Bibcode:
2002A&A...393..897R.
doi:
10.1051/0004-6361:20020943.
eISSN
1432-0746.
ISSN
0004-6361.
-
^ Kunzli, M.; North, P. (1998). "Behaviour of calcium abundance in Am-Fm stars with evolution". Astronomy and Astrophysics. 330: 651.
arXiv:
astro-ph/9710223.
Bibcode:
1998A&A...330..651K.
-
^
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.