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M. Fang

9 papers hereh-index 6483 citations14 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author7

Across the 7 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • astro-ph.GA3
  • astro-ph.EP2
same name
  • M. Fang — 64 papers, h 23
  • M. Fang — 28 papers, h 23
  • M. Fang — 13 papers, h 20
  • M. Fang — 13 papers, h 5
  • M. Fang — 6 papers, h 10
  • M. Fang — 4 papers, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20172026
most citedStar formation in IC1396: Kinematics and subcluster structure revealed by Gaia

11 citations · 12 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

Gaia24ccy: An outburst followed the footsteps of its predecessor

Koshvendra Singh, Joe P. Ninan, Zhen Guo +25

Accretion-driven outbursts in young stellar objects remain poorly understood, largely limited by a statistically small sample of closely followed-up events. This underscores the im…

astro-ph.SR2023

Stable accretion in young stars: The cases of EX Lupi and TW Hya

A. Sicilia-Aguilar, J. Campbell-White, V. Roccatagliata +8

We examine the long-term spectroscopic and photometric variability of EX~Lupi and TW~Hya, studying the presence of stable accretion and the role it plays in the observed variabilit…

astro-ph.SR2017

Millimeter Observations of the disk around GW Ori

M. Fang, A. Sicilia-Aguilar, D. Wilner +4

The GW Ori system is a pre-main sequence triple system (GW Ori A/B/C) with companions (GW Ori B/C) at ∼1 AU and ∼8 AU, respectively, from the primary (GW Ori A). The prim…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.