Q82263334

young stellar object in the constellation Perseus

Thing young_stellar_object Q82263334

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Q82263334

Summary

Q82263334 is a young stellar object^[1].

Key Facts

Q82263334's instance of is recorded as young stellar object^[2].
Q82263334's constellation is recorded as Perseus^[3].
Q82263334's spectral class is recorded as M2^[4].
Q82263334 is part of IC 348^[5].
Q82263334's catalog code is recorded as Cl* IC 348 H 228^[6].
Q82263334's catalog code is recorded as Cl* IC 348 LRL 186^[7].
Q82263334's catalog code is recorded as Cl* IC 348 LNB 23^[8].
Q82263334's catalog code is recorded as 2MASS J03444631+3211165^[9].
Q82263334's catalog code is recorded as CXOPZ 181^[10].
Q82263334's catalog code is recorded as SSTc2d J034446.3+321117^[11].
Q82263334's catalog code is recorded as CXOPZ J034446.3+321117^[12].
Q82263334's catalog code is recorded as [PSZ2003] J034446.3+321116^[13].
Q82263334's catalog code is recorded as CXOU J034446.3+321116^[14].
Q82263334's catalog code is recorded as [BNM2013] 32.03 492^[15].
Q82263334's catalog code is recorded as Gaia DR2 216702029459031552^[16].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.358'}^[17].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+24.013'}^[18].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.915'}^[19].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.369'}^[20].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.996'}^[21].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.555'}^[22].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.928'}^[23].
Q82263334's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.0498'}^[24].
Q82263334's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.5296'}^[25].
Q82263334's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.659347000'}^[26].

Body

Definition and Type

Q82263334's instance of is recorded as young stellar object^[2].

Use and Application

Q82263334 is part of IC 348^[5].

⭐ Popularity Graph

0/100 long tail

Quick Facts

Instance of young stellar object

Part of IC 348

Properties

Apparent magnitude unit: 1, amount: +17.358, unit: 1, amount: +24.013, unit: 1, amount: +20.915, unit: 1, amount: +18.369, unit: 1, amount: +13.996, unit: 1, amount: +12.555, unit: 1, amount: +11.928, unit: 1, amount: +19.0498

Catalog code Cl* IC 348 H 228, Cl* IC 348 LRL 186, Cl* IC 348 LNB 23, 2MASS J03444631+3211165, CXOPZ 181, SSTc2d J034446.3+321117, CXOPZ J034446.3+321117, [PSZ2003] J034446.3+321116, CXOU J034446.3+321116, [BNM2013] 32.03 492, Gaia DR2 216702029459031552

Constellation Perseus

Declination unit: www.wikidata.org, amount: +32.18793964881270

Declination component of proper motion unit: www.wikidata.org, amount: -7.166

Effective temperature unit: www.wikidata.org, amount: +3724

Epoch J2000.0

Imported from wholeness_audit_2026-05-02_v2

Parallax unit: www.wikidata.org, amount: +4.5296

Radial velocity unit: www.wikidata.org, amount: +14.659347000, unit: www.wikidata.org, amount: +14.659347, unit: www.wikidata.org, amount: +14.567274

Right ascension unit: www.wikidata.org, amount: +56.19296333024890

Right ascension component of proper motion unit: www.wikidata.org, amount: +4.306

Spectral class M2

Stellar rotational velocity unit: www.wikidata.org, amount: +11.07

Surface gravity unit: www.wikidata.org, amount: +13500

External References (2)

Gaia id 216702029459031552

Simbad id Cl* IC 348 LRL 186

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

[2] ↑ Q82263334 — instance of (P31): young stellar object. SIMBAD. wikidata.org.
[3] ↑ Q82263334 — constellation (P59): Perseus. wikidata.org.
[4] ↑ Q82263334 — spectral class (P215): M2. Deep MIPS observations of the IC 348 nebula: constraints on the evolutionary state of anemic circumstellar disks and the primordial-to-debris disk transition. wikidata.org.
[5] ↑ Q82263334 — part of (P361): IC 348. SIMBAD. wikidata.org.
[6] ↑ Q82263334 — catalog code (P528): Cl* IC 348 H 228. SIMBAD. wikidata.org.
[7] ↑ Q82263334 — catalog code (P528): Cl* IC 348 LRL 186. SIMBAD. wikidata.org.
[8] ↑ Q82263334 — catalog code (P528): Cl* IC 348 LNB 23. SIMBAD. wikidata.org.
[9] ↑ Q82263334 — catalog code (P528): 2MASS J03444631+3211165. SIMBAD. wikidata.org.
[10] ↑ Q82263334 — catalog code (P528): CXOPZ 181. SIMBAD. wikidata.org.
[11] ↑ Q82263334 — catalog code (P528): SSTc2d J034446.3+321117. SIMBAD. wikidata.org.
[12] ↑ Q82263334 — catalog code (P528): CXOPZ J034446.3+321117. SIMBAD. wikidata.org.
[13] ↑ Q82263334 — catalog code (P528): [PSZ2003] J034446.3+321116. SIMBAD. wikidata.org.
[14] ↑ Q82263334 — catalog code (P528): CXOU J034446.3+321116. SIMBAD. wikidata.org.
[15] ↑ Q82263334 — catalog code (P528): [BNM2013] 32.03 492. SIMBAD. wikidata.org.
[16] ↑ Q82263334 — catalog code (P528): Gaia DR2 216702029459031552. SIMBAD. wikidata.org.
[17] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+17.358'}. Do accretion discs regulate the rotation of young stars?. wikidata.org.
[18] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+24.013'}. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
[19] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+20.915'}. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
[20] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+18.369'}. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
[21] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+13.996'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[22] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+12.555'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[23] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+11.928'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[24] ↑ Q82263334 — apparent magnitude (P1215): {'unit': '1', 'amount': '+19.0498'}. Gaia Data Release 2. wikidata.org.
[25] ↑ Q82263334 — parallax (P2214): {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.5296'}. Gaia Data Release 2. wikidata.org.
[26] ↑ Q82263334 — radial velocity (P2216): {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.659347000'}. IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.

Class ancestry

[1] ↑ Q82263334 is an instance of young stellar object (Q497654) [P31, primary]. Wikidata. wikidata.org.

📑 Cite this page

Use these citations when quoting this entity in research, articles, AI prompts, or wherever provenance matters. We aggregate Wikidata + Wikipedia + authoritative open-data sources; the stitched, scored, cross-referenced view is what 4ort.xyz contributes.

APA 4ort.xyz Knowledge Graph. (2026). Q82263334. Retrieved May 7, 2026, from https://4ort.xyz/entity/q82263334

MLA “Q82263334.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q82263334.

BibTeX

@misc{4ortxyz_q82263334_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q82263334}}, year = {2026}, url = {https://4ort.xyz/entity/q82263334}, note = {Accessed: 2026-05-07}}

LLM prompt

According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q82263334 — https://4ort.xyz/entity/q82263334 (retrieved 2026-05-07)

Canonical URL: https://4ort.xyz/entity/q82263334 · Last refreshed: May 7, 2026